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- {{Short description|Remains of a galaxy merger in the Milky Way}} ...om the dwarf galaxy, the data taken from a simulated merger with the Milky Way with similar properties to the one believed to have occurred. ...11 KB (1,527 words) - 23:34, 11 November 2024
- ...likely between 1 and 3). All of the data used were gathered from the Milky Way, and specifically the solar neighborhood. ...author2=Evans, Neal II | date = 2012 | title = Star Formation in the Milky Way and Nearby Gaalxies | journal = Annual Review of Astronomy & Astrophysics | ...3 KB (440 words) - 22:16, 27 March 2024
- {{Short description|Coherent, wave-shaped gaseous structure in the Milky Way}} ...in the Galaxy|url=https://www.livescience.com/radcliffe-wave-largest-milky-way-structure.html|website=livescience.com}}</ref><ref name=":0" /> ...10 KB (1,415 words) - 21:58, 30 September 2024
- # the mass is distributed in the same way as the observed stars. ...e the mass of the [[supermassive black hole]] at the center of the [[Milky Way]] galaxy.<ref>{{Cite journal ...4 KB (593 words) - 08:47, 13 December 2024
- ...C 6496''' is a [[globular cluster]] which is in the direction of the Milky Way's [[galactic bulge]] based on observations collected with the WFPC2 on boar ...an A. | last2=Bridges | first2=Terry | title=Accreted versus in situ Milky Way globular clusters | journal=[[Monthly Notices of the Royal Astronomical Soc ...6 KB (757 words) - 14:40, 6 September 2024
- ...the most commonly used tools for Galactic population analysis of the Milky Way. The diagrams use abundance ratios normalised to the Sun, (placing the Sun ...Metallicity Distribution Functions and the Chemical Structure of the Milky Way Disk |journal=The Astrophysical Journal |volume=808 |issue=2 |pages=132|doi ...9 KB (1,360 words) - 11:45, 2 September 2024
- === Milky Way dark matter halo === ...ft|thumb|217x217px|Artistic rendition of dark matter halo around the Milky Way. Jeans Equation simulations place limits on the size of this halo]] ...12 KB (1,782 words) - 12:49, 4 February 2025
- ...ual to the mass of the supermassive black hole. In the case of the [[Milky Way]], the mass of the supermassive black hole is about 4 million [[Solar mass] ...rst3=R. |date=2018-01-01 |title=The distribution of stars around the Milky Way's central black hole. III. Comparison with simulations |url=https://ui.adsa ...12 KB (1,740 words) - 18:36, 20 September 2023
- ...the closest [[supermassive black hole]]s including the ones in the [[Milky Way]], [[Andromeda Galaxy|M31]], [[Messier 32|M32]], [[Messier 81|M81]], [[Mess ...6 KB (868 words) - 23:20, 21 September 2024
- ...scription|Large collections of gas found in the galactic halo of the Milky Way}} ...n HVCs around the Andromeda Galaxy, but this treats the phenomena as Milky Way objects|date= April 2013}} ...26 KB (4,077 words) - 18:02, 14 November 2024
- ...ffei 1 is situated at an estimated distance of 3–4 Mpc from the Milky Way. It may be the closest giant elliptical galaxy. ...i 1 lies in the [[Zone of Avoidance]] and is heavily obscured by the Milky Way's [[star]]s and [[cosmic dust|dust]]. If it were not obscured, it would be ...15 KB (2,150 words) - 07:48, 1 November 2024
- ...[[stars]] from the [[Milky_Way#Composition_and_structure|disc of the Milky Way]], it is very difficult [[Celestial body|object]] to study<ref name="Carrar ...4 KB (474 words) - 04:53, 5 April 2021
- ...th. If the string should be raised {{convert|1|m}} off the ground, all the way along the equator, how much longer would the string be? ...is irrelevant, and may be anything from the size of an atom to the [[Milky Way]] — the result depends only on the amount it is raised. Moreover, as ...5 KB (782 words) - 03:27, 18 February 2025
- ...tions from stars on other orbits. Assuming that the [[Sagittarius A*|Milky Way black hole]] is maximally rotating, its rotational influence radius is abou ...4 KB (612 words) - 08:42, 9 November 2024
- ...600 [[parsec|pc]]) from [[Earth]], in an isolated area of the [[Milky Way]].<ref name="nasa-sa" /> ...4 KB (542 words) - 05:47, 7 November 2024
- ...p>9</sup> [[Solar mass|<var>M</var><sub>☉</sub>]] (Compared to the [[Milky Way]]'s mass of about 10<sup>12</sup> [[Solar mass|<var>M</var><sub>☉</sub>]]). ...5 KB (685 words) - 16:56, 31 March 2024
- ...tle=Luminosities of carbon-rich asymptotic giant branch stars in the Milky Way |author = Guandalini, R. |author2 = Cristallo, S. |journal = Astronomy & As ...4 KB (602 words) - 05:15, 18 November 2024
- ...from a variety of sources such as the Sun, the [[Solar System]], the Milky Way galaxy, or even further beyond.<ref name=":1">{{Cite journal |last=Kajita | ...ift]] correction, and sources of high energy outside the [[Milky Way|Milky Way Galaxy]].<ref name=":0" /> ...16 KB (2,400 words) - 10:42, 10 February 2025
- ...n disk of galaxy that is about 3 billion light years away from the [[Milky Way]]. They used the [[William Herschel Telescope]] to observe this galaxy, and ...5 KB (791 words) - 05:22, 17 November 2024
- ...the infrared surface brightness technique: I. The ''p''-factor, the Milky Way relations, and a universal ''K''-band relation |journal=Astronomy & Astroph ...Hertzsprung]] determined the distances of several Cepheids in the [[Milky Way]] and that, with this calibration, the distance to any Cepheid could then b ...20 KB (2,865 words) - 01:25, 16 February 2025