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  • {{Short description|Spiral galaxy in the constellation Cetus}} | type=[[Intermediate spiral galaxy|SAB(s)ab]] ...
    6 KB (804 words) - 00:59, 27 November 2024
  • ...ge. Points are labelled by galaxy name; all points in this diagram are for galaxies that have a clear, [[Kepler's laws of planetary motion|Keplerian]] rise in ...Black holes and galaxy evolution | volume = 197 | book-title = Dynamics of Galaxies: from the Early Universe to the Present | publisher = [[Astronomical Societ ...
    13 KB (1,932 words) - 18:57, 1 March 2025
  • | names = [[Principal Galaxies Catalogue|PGC]] 9892, [[Uppsala General Catalogue Addendum|UGCA]] 034<ref n ...nown to belong to a separate group, the [[IC 342/Maffei Group]]. It was [[galaxies named after people|named]] after [[Paolo Maffei]], who discovered it and th ...
    15 KB (2,150 words) - 07:48, 1 November 2024
  • ...y Press, 2012.</ref> [[Newtonian fluid]]s, and the [[fluid dynamics]] of [[galaxies]]. ...d caused by spiral density waves in the [[Galactic disc|stellar discs]] of galaxies. Since supersonic motions almost always involve [[shock wave]]s, shock wave ...
    11 KB (1,746 words) - 18:28, 6 August 2024
  • ...y. They have been observed in the Milky Way's halo and within other nearby galaxies. ...s are probably spawned by interactions between the Milky Way and satellite galaxies, such as the [[Magellanic Clouds|Large and Small Magellanic Clouds]] (LMC a ...
    26 KB (4,077 words) - 18:02, 14 November 2024
  • ...y|satellites]] as well as the internal kinematics of more distant [[Galaxy|galaxies]]. Measurement of the kinematics of stars in different subcomponents of the ...the influence of [[gravity]]. Stellar-dynamical models of systems such as galaxies or star clusters are often compared with or tested against stellar-kinemati ...
    61 KB (8,592 words) - 01:54, 20 January 2025
  • ...agazine)|Wired]] |accessdate=10 January 2023 }}</ref><ref name=FPI_1/> Pea galaxies are so-named because of their small size and greenish appearance in the ima "Pea" galaxies were first discovered in 2007 by the volunteer [[citizen scientists]] withi ...
    100 KB (14,565 words) - 21:06, 19 February 2025
  • ...en used to clarify many characteristics of our galaxy, such as the local [[spiral arm]] structure and the Sun's distance from the [[galactic plane]].<ref nam ...more are known in the [[Magellanic Clouds]], with more discovered in other galaxies;<ref>{{cite journal|bibcode=2003ASPC..298..237S|title=Cepheids: Observation ...
    40 KB (5,621 words) - 10:43, 14 January 2025