Search results

Jump to navigation Jump to search
  • spiral galaxy. Def. a galaxy having a smooth, featureless light-profile is called an elliptical galaxy. Def. a galaxy that like spiral galaxies has a flat...
    87 KB (10,378 words) - 14:50, 26 January 2023
  • define a galaxy. While it is part of the astronomy course principles of radiation astronomy, it is also independent. Some suggested galaxy entities to...
    11 KB (1,266 words) - 06:05, 18 August 2022
  • towards a coherent theory of galaxy evolution, the American astronomer Edwin Hubble, developed a classification scheme of galaxies in 1926. The image centered...
    4 KB (397 words) - 04:13, 23 January 2020
  • name for the galaxy we live in. It is a member of the Local Group of galaxies. Here's a theoretical definition: Def. a large spiral galaxy that includes...
    38 KB (4,463 words) - 02:39, 17 August 2023
  • Drake et al. (1969)." Def. occurring between galaxies is called intergalactic. Def. originating outside the Milky Way galaxy or outside of a galaxy is called...
    101 KB (12,056 words) - 04:01, 30 November 2020
  • The spiral galaxy NGC 3319 in the image on the right is about 47 million light-years away. Def. "[a]ny of the collections of many millions of stars .....
    38 KB (4,663 words) - 04:18, 18 December 2019
  • he was able to conclusively show that M31, was indeed far beyond this galaxy. We now know it to be 2.2 million light-years away. A globular cluster is...
    3 KB (404 words) - 04:17, 6 January 2020
  • is the image on the right. "The invisible cloud is plummeting toward our galaxy at nearly 700,000 miles per hour." "This composite image shows the size...
    112 KB (13,361 words) - 02:39, 1 October 2022
  • the bright object seen slightly below and to the right of the galaxy's centre. The galaxy and its bright supernova were observed on the nights of 16, 19...
    16 KB (1,870 words) - 15:30, 19 April 2023
  • et al. (18 December 2003). Galaxy IRAS F00183-7111. Pasadena, California USA: Caltech. http://www.spitzer.caltech.edu/images/1098-ssc2003-06h-Galaxy-IRAS-F00183-7111...
    204 KB (23,126 words) - 11:29, 6 June 2023
  • effort, in a lecture/article format, to describe the Milky Way, our home galaxy, often as applied in the performance of radiation astronomy. You are free...
    5 KB (454 words) - 22:49, 21 January 2019
  • central galaxy, NGC 1275." "And the bay's shape doesn't match those predicted by computer models that simulate normal gas sloshing." "Galaxy cluster mergers...
    26 KB (3,383 words) - 11:08, 6 June 2023
  • Kupfer; U. Heber; A. Irrgang; B. Wang; Z. Liu et al. (2015-03-06). "The fastest unbound star in our Galaxy ejected by a thermonuclear supernova". Science...
    82 KB (9,369 words) - 13:37, 25 January 2024
  • shows the Andromeda galaxy, a neighbor to our Milky Way galaxy. The main image (top) highlights the contrast between the galaxy's choppy waves of dust...
    54 KB (6,166 words) - 11:13, 6 June 2023
  • such stars are present in the old stellar populations of all galaxies (but see Foss et al. 1991), there is good reason to believe that Type Ia supernovae...
    46 KB (5,402 words) - 21:28, 23 August 2021
  • VV340A is the face-on galaxy, and VV340B is the edge-on galaxy. In both images of UGC 9618, 50 mm corresponds to 2.4' of arc. The galaxy on edge is 16 mm in...
    15 KB (1,884 words) - 04:27, 20 August 2022
  • Fischer et al. (December 10, 2000). "The very red afterglow of GRB 000418: Further evidence for dust extinction in a gamma-ray burst host galaxy". The Astrophysical...
    95 KB (12,068 words) - 15:32, 8 February 2024
  • most powerful quasars have luminosities thousands of times greater than a galaxy such as the Milky Way. High-resolution images of quasars, particularly from...
    47 KB (6,162 words) - 17:02, 15 January 2022
  • medium is the matter that exists in the space between the star systems in a galaxy. At right is a visual negative of the LW Cassiopeia Nebula (ISM). Within...
    100 KB (11,031 words) - 19:59, 26 August 2022
  • survey included: Detection of galaxies in the "Zone of Avoidance", a strip of sky obscured in visible light by our own galaxy, the Milky Way. Detection of...
    17 KB (2,299 words) - 22:20, 21 February 2019
  • light-years wide, it is only 8,000 light-years from our Galaxy's disk. It is careening toward our Galaxy at more than 150 miles per second, aimed to strike...
    102 KB (11,895 words) - 19:07, 4 December 2021
  • Cirasuolo; J.S. Dunlop; J.A. Peacock; D. Farrah et al. (April 2010). "X-ray groups and clusters of galaxies in the Subaru-XMM Deep Field". Monthly Notices...
    135 KB (16,395 words) - 23:08, 12 November 2022
  • the interstellar medium (the hydrogen and helium gas that permeates the galaxy) by the solar wind. Although electrically neutral atoms from interstellar...
    11 KB (1,308 words) - 18:11, 22 August 2022
  • of light-years, depending on the size of the associated object such as a galaxy. Once an entity, source, or object [such as a corona or coronal cloud] has...
    103 KB (11,737 words) - 11:08, 6 June 2023
  • jets in the Galaxy” Annual Review of Astronomy and Astrophysics, 37, 409 Mirabel, I.F. & Rodríguez, L.F. (1998) “Microquasars in our Galaxy” Nature, 392...
    8 KB (1,163 words) - 03:13, 16 October 2020
  • Shintaro Koshida et al. (March 1, 2006). "Reverberation Measurements of the Inner Radius of the Dust Torus in Nearby Seyfert 1 Galaxies". The Astrophysical...
    85 KB (10,704 words) - 04:11, 5 December 2020
  • on the right record emission events for AT2018cow. The first shows the galaxy Z 137-068. The second down on the right has two markers ending close to...
    6 KB (664 words) - 04:46, 2 January 2021
  • produced a matched trio of images of the central region of our Milky Way galaxy. Each image shows the telescope's different wavelength view of the galactic...
    48 KB (6,001 words) - 17:39, 15 January 2022
  • the human eye." "[H]igh-resolution (0.1") observations of the Seyfert 2 galaxy NGC 5728 with the Hubble Space Telescope", in the images at right, show...
    14 KB (1,592 words) - 22:15, 14 November 2022
  • places this star at the high temperature end of the cyan band. "The spiral galaxy, Messier 83, NGC 5236 [is shown in the image at right]. [The t]ri-colour...
    4 KB (318 words) - 05:26, 24 September 2021
  • (Alcock et al. 1999)." "It is important to study the stellar populations of nearby galaxies like the LMC in order to understand the processes of galaxy evolution...
    100 KB (13,091 words) - 22:40, 22 April 2022
  • uncommonly high speed (about 130 km/s (81 mi/s)) relative to the Milky Way galaxy's ambient gas. Mira itself is seen as a small white dot inside a blue bulb...
    40 KB (4,783 words) - 21:03, 30 November 2020
  • called a galaxy. Def. any galaxy, considerably smaller than the Milky Way, that has only several billions of stars is called a dwarf galaxy. Def. a small...
    116 KB (13,352 words) - 12:24, 6 June 2023
  • rays that originate predominantly from super nova explosions within our galaxy. Interactions between these high energy cosmic rays and the Earth's atmosphere...
    113 KB (13,574 words) - 00:02, 18 April 2023
  • the only nearby galaxy to show evidence for superluminal motion." "This discovery goes a long way towards confirming that radio galaxies, quasars and exotic...
    21 KB (2,446 words) - 03:42, 23 November 2020
  • in the photo are supermassive black holes, which lie at the hearts of galaxies and contain 100,000 to 10 billion times the mass of the sun." "It can be...
    10 KB (1,358 words) - 01:55, 6 November 2020
  • trigonometric parallax of their movements relative to background stars or galaxies that are immobile within the resolution of the telescope used. When X-ray...
    99 KB (13,935 words) - 04:03, 15 December 2020
  • important to study the stellar populations of nearby galaxies in order to understand the processes of galaxy 17 True or False, A new cosmogony predicts that...
    14 KB (995 words) - 22:32, 29 April 2020
  • a very low mass M-type star which make up about 76% of all stars in our galaxy, the Milky Way. Other stars with larger masses, about ten times that of...
    9 KB (1,256 words) - 02:01, 5 December 2020
  • group of galaxies after HCG 92." "To that end we used the very compact 375-m array of the Australia Telescope Compact Array (ATCA; Frater et al. 1992)1...
    35 KB (3,975 words) - 19:52, 24 January 2022
  • et al., 1981) may indicate material originating from WC stars. Moreover, as there is a strong gradient in the distribution of WC stars in the Galaxy, a...
    107 KB (13,375 words) - 02:32, 20 April 2022
  • witnessed a supernova soon after it exploded in the Messier 82, or M82, galaxy. Telescopes across the globe and in space turned their attention to study...
    103 KB (13,296 words) - 13:37, 25 January 2024
  • are multiple images of the same galaxy, duplicated by the gravitational lens effect of the cluster of yellow galaxies near the middle of the photograph...
    27 KB (3,053 words) - 19:18, 4 December 2021
  • that exist on the edges of galaxies." "Lying 50 000 light-years from Earth, in the outer reaches of our Milky Way galaxy, NGC 6934 is home to some of...
    18 KB (2,114 words) - 22:51, 29 April 2020
  • astro-ph / 0604076 v1, 4 Apr 2006. Joe Wolf at al. Accurate masses for dispersion-supported galaxies. Monthly Notices of the Royal Astronomical Society...
    28 KB (4,785 words) - 00:58, 5 April 2023
  • old stellar systems, such as globular clusters, spiral galaxy bulges and elliptical galaxies. They are prominent on ultraviolet images. The hot subdwarfs...
    42 KB (4,894 words) - 19:25, 14 November 2022
  • number of dwarf galaxies surrounding the Galaxy like the electrons in the oxygen atom. The tight group of galaxies, consisting of the Galaxy and the Large...
    52 KB (8,000 words) - 00:57, 5 April 2023
  • Ota; Mamoru Doi; Masaru Hamabe et al. (August 20, 2004). "Subaru Deep Survey. VI. A Census of Lyman Break Galaxies at z ≃ 4 and 5 in the Subaru Deep Fields:...
    94 KB (9,934 words) - 16:43, 2 July 2023
  • first galaxies, the way galaxies change over time, and the processes that have generated the variety of structures observed in nearby galaxies. It is...
    96 KB (11,376 words) - 18:35, 7 September 2021
  • BSGMODEL: The Bahcall-Soneira Galaxy Model Bahcall, J. N. http://ascl.net/9904.001 BSGMODEL: The Bahcall-Soneira Galaxy Model Bahcall, J. N. http://ascl...
    22 KB (3,195 words) - 09:15, 26 October 2019
  • assessed using the Hubble scheme: Probably the earliest classification of galaxies "is based on the forms of the photographic images." "About 3 per cent are...
    8 KB (832 words) - 00:41, 30 April 2020
  • down-flows seen in the STIS spectra." "One out of a million stars in our galaxy is a supergiant and fewer yet are cool supergiants. Not only is Betelgeuse...
    66 KB (8,271 words) - 22:07, 14 November 2022
  • The "star formation process happens very quickly and in regions of the Galaxy that are difficult to study observationally." Nonaxisymmetric "magnetic...
    91 KB (11,272 words) - 05:18, 6 December 2020
  • Astrophysics: 19. http://arxiv.org/abs/1403.1275. Retrieved 2014-04-17.  The Daily Galaxy via the Alma Observatory (March 7, 2014). Beta Pictoris: A Young, Violent...
    95 KB (12,008 words) - 19:39, 12 May 2023
  • travel with velocities so high that they exceed the escape velocity of the Galaxy." "A multinational team of astronomers led by Dr Stephan Geier from the...
    19 KB (1,684 words) - 15:18, 22 August 2020
  • analogue of electrons at the level of galaxies. However the ratio of the minimum galaxy mass of a normal galaxy to the mass of a typical globular cluster...
    117 KB (19,391 words) - 00:56, 5 April 2023
  • much larger gravitationally bound structure, such as a star cluster or a galaxy. Historically, stars have been important to civilizations throughout the...
    82 KB (9,515 words) - 16:42, 8 January 2023
  • JWST will be in order to understand the initial stages of the universe, galaxy formation as well as the formations of stars and planets, and the origins...
    11 KB (1,372 words) - 13:35, 2 February 2021
  • Van Eck et al. 2003). This has modified the estimates of the amount of s-lead produced in the Galaxy before the birth of the Sun (Gallino et al 1998), and...
    98 KB (11,466 words) - 05:11, 6 December 2020
  • size of Jupiter. Stars/Nova-likes Michelle Starr (12 August 2019). "Our Galaxy's Supermassive Black Hole Has Emitted a Mysteriously Bright Flare". Science...
    26 KB (2,951 words) - 19:30, 14 November 2022
  • binaries and multiple gaseous object systems including clusters, galaxies, and galaxy clusters. Stellar classification is a classification of stars based...
    95 KB (12,456 words) - 20:14, 14 November 2022
  • the interstellar medium (the hydrogen and helium gas that permeates the galaxy) by the solar wind. Although electrically neutral atoms from interstellar...
    103 KB (12,867 words) - 10:38, 6 June 2023
  • galaxies for each redshift bucket with a uniform distribution, and computing the number of visible galaxies (those not covered by foreground galaxies)...
    13 KB (1,983 words) - 21:11, 25 July 2021
  • increase in the intensity of high-energy electrons from elsewhere in the galaxy diffusing into our solar system from outside ... [while] the [solar] wind...
    103 KB (12,420 words) - 08:48, 30 May 2023
  • keV stand for 103 electron volts. Compact groups of galaxies are tight associations of galaxies. Their compactness suggests extremely short crossing...
    62 KB (6,288 words) - 08:00, 5 January 2022
  • such stars are present in the old stellar populations of all galaxies (but see Foss et al. 1991), there is good reason to believe that Type Ia supernovae...
    116 KB (15,684 words) - 05:12, 6 December 2020
  • found only electrons streaming into the heliosphere from elsewhere in the galaxy. Usually the separation of charge carriers, such as electrons and protons...
    57 KB (7,290 words) - 23:27, 30 November 2020
  • responsible for the production of B and Be throughout the history of the Galaxy." Def. "an energetic particle originating outside our solar system" is called...
    46 KB (5,524 words) - 22:25, 22 June 2022
  • Second, they are dependent on our special place at the edge of the Milky Way galaxy and did not suggest the radiation is isotropic. Moreover, they would yield...
    26 KB (4,002 words) - 04:03, 12 September 2020
  • massive galaxies; these data also suggest the presence of unseen mass." "Even if gaseous bound systems of galactic mass can form, the types of galaxy they...
    70 KB (8,896 words) - 05:09, 30 June 2022
  • process that provided light neutron-capture elements in the very early Galaxy." "A comparison of the heavy-element abundance distribution in [AG Draconis]...
    99 KB (12,612 words) - 01:24, 23 August 2022
  • that the farther galaxies were from us, the faster they statistically tend to be traveling away from us. This means that the galaxies tend to be spreading...
    15 KB (1,981 words) - 04:15, 13 May 2022
  • Analytical astronomy Cosmogony Cratering Electric orbits Electron beam heating Galaxies Intergalactic medium Locating the Sun Magnetic field reversal Meteorites...
    20 KB (2,101 words) - 08:48, 30 May 2023
  • 1051/0004-6361:20020806.  Francesca Matteucci (2001). The Chemical Evolution of the Galaxy. Astrophysics and Space Science Library. 253. Springer Science & Business...
    30 KB (3,770 words) - 01:37, 1 December 2020
  • from Earth to the Moon in 24 minutes!" "NGC 6302 lies within our Milky Way galaxy, roughly 3,800 light-years away in the constellation Scorpius. The glowing...
    61 KB (6,701 words) - 03:54, 30 June 2022
  • within the Milky Way that the Sun appears to be "chasing" as it orbits the galaxy. The general direction of the solar apex is southwest of the star Vega near...
    103 KB (12,605 words) - 08:48, 30 May 2023
  • Analytical astronomy Cosmogony Cratering Electric orbits Electron beam heating Galaxies Intergalactic medium Locating the Sun Magnetic field reversal Meteorites...
    8 KB (813 words) - 17:49, 11 August 2022
  • be due to a larger star companion. First astronomical X-ray source/Quiz Galaxies/Quiz Radiation astronomy/Quiz Star fission/Quiz Stars/Quiz Stellar active...
    4 KB (275 words) - 02:34, 5 February 2020
  • Analytical astronomy Cosmogony Cratering Electric orbits Electron beam heating Galaxies Intergalactic medium Locating the Sun Magnetic field reversal Meteorites...
    24 KB (3,248 words) - 16:23, 29 August 2022
  • [asymptotic giant branch] AGB stars that formed early in the history of the Galaxy, and that therefore have very low abundances of elements heavier than helium...
    45 KB (5,483 words) - 16:20, 8 January 2021
  • to indicate the masses of other stars, as well as clusters, nebulae and galaxies. It is equal to the mass of the Sun, about two nonillion kilograms: M ⊙...
    39 KB (4,841 words) - 08:49, 30 May 2023
  • p + p + p + A The secondary antiprotons (p) then propagate through the galaxy, confined by the galactic magnetic fields. Their energy spectrum is modified...
    38 KB (4,431 words) - 10:35, 6 June 2023
  • that support the existence of dark matter - article by Douglas Clowe, et al. (2006) DAMA/NaI - laboratory experiment attempting to detect dark matter...
    2 KB (151 words) - 04:51, 17 July 2018
  • the interstellar medium (the hydrogen and helium gas that permeates the galaxy) by the solar wind. Although electrically neutral atoms from interstellar...
    97 KB (10,469 words) - 08:48, 30 May 2023
  • with an estimate that the abundance of lithium at the beginning of the galaxy was: NLi = (11.2 ± 3.8) × 10−11 NH where NH is the abundance of hydrogen...
    59 KB (6,859 words) - 04:24, 30 June 2022
  • to or been caught up to by a red or brown dwarf star in orbit around the galaxy. Earth's orbit around the Sun at some 51° to the galactic plane may have...
    99 KB (11,415 words) - 07:37, 30 May 2023
  • star formation, which plays host to some of the highest-mass stars in our galaxy, is an ideal arena in which to study the interactions between these young...
    24 KB (3,338 words) - 07:24, 24 August 2022
  • nitrogen/oxygen (N/O) abundance gradients. Surveys of H II regions in spiral galaxies have suggested that N/O abundance ratios increase from outer-arm nebulae...
    47 KB (4,989 words) - 06:39, 4 February 2024
  • pleasing stimuli conform to this ratio. The golden ratio can be found in galaxies, the natural environment and even within the human body, and has been utilised...
    30 KB (3,827 words) - 20:58, 4 March 2021
  • Kratz, K.-L.; Frebel, A. et al. (2009). "The end of nucleosynthesis: Production of lead and thorium in the early galaxy". The Astrophysical Journal (The...
    162 KB (18,268 words) - 14:40, 14 September 2022
  • mysteriously connected to the behavior of an obscure atom in a distant galaxy billions of years ago. The third loophole was a surprise for us. In an early...
    46 KB (6,266 words) - 04:52, 15 June 2022
  • carbon stars found in globular clusters and some dwarf spheroidal (dSph) galaxies (Harding 1962). Among these, at high Galactic lat- itudes, warm carbon...
    25 KB (3,483 words) - 05:46, 20 June 2021
  • than 46,000 variable stars in the Milky Way, as well as 10,000 in other galaxies, and over 10,000 'suspected' variables. SIMBAD recognizes some 36 types...
    32 KB (3,412 words) - 22:09, 14 November 2022
  • increase in the intensity of high-energy electrons from elsewhere in the galaxy diffusing into our solar system from outside ... [while] the [solar] wind...
    70 KB (8,537 words) - 11:08, 6 June 2023
  • be 2 e- cm-2 s-1 diffusing into our solar system from elsewhere in the galaxy. Each of these electrons has an energy of 10 MeV. Φ e − = 2 e − ⋅ c m −...
    38 KB (5,671 words) - 08:48, 30 May 2023
  • sense the presence of a planet." "It is the most common type of star in the galaxy — over 70 percent of Milky Way stars are like this dim, M dwarf star. Though...
    100 KB (11,456 words) - 04:11, 5 December 2020
  • et al., 1981) may indicate material originating from WC stars. Moreover, as there is a strong gradient in the distribution of WC stars in the Galaxy, a...
    184 KB (22,557 words) - 23:21, 8 June 2022
  • spectral type. Red dwarfs are by far the most common type of star in the Galaxy, at least in the neighborhood of the Sun. Proxima Centauri, the nearest...
    93 KB (4,127 words) - 03:19, 5 October 2021
  • stars). http://adsabs.harvard.edu/abs/2001JRASC..95...32L.  R. O. Gray, et al. (July 2006). "Contributions to the Nearby Stars (NStars) Project: Spectroscopy...
    24 KB (2,945 words) - 19:53, 9 August 2022
  • Constellations and Their Legends, p. 66 (ISBN 9780521544153). Hubrig, S.; et al. (June 2001). "Search for low-mass PMS companions around X-ray selected late...
    26 KB (3,580 words) - 04:49, 28 August 2022
  • (June 19, 1989). 3-dimensional particle-in-cell simulations of spiral galaxies. Heidelberg, Federal Republic of Germany: Kluwer Academic Publishers. pp...
    69 KB (8,911 words) - 15:31, 29 November 2020
  • the collimation of relativistic jets in the gravitomagnetic fields of galaxies, active galactic nuclei and rapidly rotating stars (eg, jet accreting neutron...
    26 KB (3,588 words) - 16:41, 21 November 2023
  • or No, The most frequently preferred standard candle for distances to galaxies is the Type-II supernova. 6 Complete the text: 7 Which of the following...
    5 KB (343 words) - 13:37, 25 January 2024
  • into spherical trigonometry under the stimulus of astronomical calculation. Al Farghani (d 861) first calculated longitudes and wrote down the elements of...
    9 KB (942 words) - 22:43, 29 March 2019
  • increase in the intensity of high-energy electrons from elsewhere in the galaxy diffusing into our solar system from outside ... [while] the [solar] wind...
    46 KB (5,262 words) - 20:49, 30 November 2020
  • extracted from the Lake Ledro, located in the province of Trento (Joannin et al. 2014)." Radiocarbon "data indicate that the New Kingdom of Egypt started...
    103 KB (11,440 words) - 22:15, 9 June 2022
  • combine these objects to form more complex objects; from electrons to galaxies, while still retaining the underlying attributes (of mass, wavelength,...
    32 KB (2,563 words) - 12:59, 15 March 2024
  • This beautiful galaxy is tilted at an oblique angle to our line of sight, giving a "birds-eye view" of the spiral structure. Credit: Hubble data: NASA...
    5 KB (464 words) - 00:28, 14 January 2019
  • explain by clusters of neutron stars the phenomena in the central parts of galaxies, attributed to black holes of large masses. In the present time the main...
    98 KB (16,511 words) - 00:57, 5 April 2023
  • had been down there for 34 days when he had been gone for 59 (Halberg et al, 1970). For something so seemingly important it is surprising how easily time...
    30 KB (4,112 words) - 06:54, 22 August 2020
  • spiral waves are to account for them (akin to the spiral density waves in galaxies). Studied briefly by a Pioneer mission it has been much more extensively...
    59 KB (7,006 words) - 06:39, 30 May 2023
  • within the Milky Way that the Sun appears to be "chasing" as it orbits the galaxy." "The general direction of the solar apex is southwest of the star Vega...
    104 KB (12,577 words) - 15:07, 20 March 2021
  • a circular path at a radius of 16 light years through the space of our galaxy, then according to our time calculation he passes by our solar system every...
    20 KB (2,599 words) - 22:33, 23 March 2024
  • million from endorsements on top of a $7 million salary from the Los Angeles Galaxy and AC Milan. A perfect illustration of power laws and superstar economics...
    55 KB (8,472 words) - 05:08, 17 December 2022
  • the graviton field, reaching our Universe. The effects of redshift of the galaxy spectra and the attenuation of emission from distant supernovae can be explained...
    94 KB (15,300 words) - 01:43, 5 April 2023
  • huge cryometeor that impacted on Earth billions of years ago [Morbidelli et al., 2000]." "Schwerdtfeger (1970, p. 294) notes "With reference to Antarctica...
    173 KB (20,361 words) - 17:38, 13 October 2022
  • 10-20K dust in the interstellar medium in the Milky Way galaxy, and in distant starburst galaxies. Telescopes operating in this band include the James Clerk...
    114 KB (10,943 words) - 00:58, 31 August 2022
  • occur in dusty regions present in the old stellar populations of all galaxies they have characteristic mottling they lack hydrogen lines in their optical...
    5 KB (365 words) - 13:37, 25 January 2024
  • Constellations and Their Legends, p. 66 (ISBN 9780521544153). Hubrig, S.; et al. (June 2001). "Search for low-mass PMS companions around X-ray selected late...
    26 KB (3,551 words) - 08:50, 11 June 2021
  • and the Local Group". In F. Combes, Keiichi Wada. Mapping the Galaxy and Nearby Galaxies. Springer. pp. 19–20. ISBN 0387727671. http://books.google.com/...
    84 KB (10,998 words) - 23:23, 27 January 2024
  • unseen mass a bubble in space range of masses of galaxies hot neutrinos Einstein-de-Sitter 'flat' universe the cosmological density parameter Ω...
    7 KB (459 words) - 23:45, 22 January 2020
  • appealing voice, "low and sweet, a very excellent thing in woman" — what a galaxy was there, all taking the town by storm at the same moment, and many others...
    193 KB (31,673 words) - 21:37, 27 March 2021
  • sharper and eventually when a formed universe (with gravitational clusters, galaxies, etc.) is close enough to an early state universe the early state universe...
    26 KB (4,213 words) - 11:39, 13 April 2020
  • we have travel via hyperspace, and then we can travel from one end of a galaxy to another. Hyperspace works around the problem that Milky Way is approximately...
    180 KB (27,119 words) - 13:53, 15 February 2024
  • System OpenStax: Astronomy Harper College Astronomy AST 115 Stars and Galaxies OpenStax: Astronomy Harper College Astronomy ASTR 104 Astronomy of Planets...
    113 KB (31 words) - 01:38, 14 September 2018
  • right now,” he said. “It has to be something that’s, that’s out of our galaxy, it just has to be, if in fact it is real.” Elizondo also dismissed those...
    192 KB (28,813 words) - 19:37, 28 December 2021
  • attracted nearby matter and thus grew even denser, forming gas clouds, stars, galaxies, and the other astronomical structures observable today. Eventually the...
    67 KB (8,123 words) - 12:10, 14 February 2024
  • adiaŭ (adi') adi' the wellbeing ali' other (ali') 〔 to_or_toward- "i" 〕 〔 "al" -proform 〕 (ali') (ali') anti' the opposed 〔 "ant" -proform 〕 ati' ten to...
    529 KB (0 words) - 11:42, 9 May 2014