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{{Short description|Measure of the projected clustering of galaxies}} ....edu/level5/March04/Jones/Jones5_2.html|title=B. The correlation function: galaxies|access-date=2021-06-09}}</ref> ...

* Star-forming BzK (sBzK) galaxies satisfy: <math> BzK \equiv (z-K)_{AB} - (B-z)_{AB} \geq -0.2</math> * Passive BzK (pBzK) galaxies satisfy: <math> BzK < -0.2</math> and <math>(z-K)_{AB} > 2.5</math> ...

...pal Galaxies Catalogue|PGC]] 024836,<ref name="ned" /> [[Atlas of Peculiar Galaxies|APG]] 7<ref name="simbad" /> ...ed in his [[Atlas of Peculiar Galaxies]] under the category of 'split arm' galaxies.<ref>{{cite web ...

..., Walter|title = A simple model for the distribution of light in spherical galaxies|journal = Monthly Notices of the Royal Astronomical Society|volume = 202|pa ...uristically from the observation that the brightness profiles of spherical galaxies seem to run as <math>r^{-3}</math> and <math>r^{-1}</math> in at least some ...

{{Short description|Triplet of galaxies in the constellation Virgo}} ..., [[Principal Galaxies Catalogue|PGC]] 52130, [[Morphological Catalogue of Galaxies|MCG]]+01-37-034, [[Sloan Digital Sky Survey|SDSS]]&nbsp;J143506.38+052124.5 ...

...system (e.g. [[galaxy|galaxies]], [[Galaxy groups and clusters|clusters of galaxies]], etc.).<ref>{{cite arXiv |first=C. |last=Keeton |date=June 2002 |title=A ...

...ned the connection between surface gas density and SFR for a larger set of galaxies to estimate a value of <math>n = 1.4 \pm 0.15</math>.<ref name="kennicutt98 ...bert C. Jr. | date = 1998 | title = The Global Schmidt Law in Star-forming Galaxies | journal = The Astrophysical Journal | volume = 498 | issue = 2| pages = 5 ...

...utral and dense molecular regions in the [[interstellar medium]] inside of galaxies. Moreover, gas throughout space is [[turbulent]] implying it has density st ...

| names = MCG -01-05-005, [[Principal Galaxies Catalogue|PGC]] 5766<ref name="ned" /> ...t9=Tod R.|last10=Richstone|first10=Douglas|title=The Centers of Early-Type Galaxies with HST. IV. Central Parameter Relations.|journal=The Astronomical Journal ...

...p]] of galaxies, which is a member of the [[Virgo II Groups]], a series of galaxies and [[galaxy cluster]]s strung out from the southern edge of the [[Virgo Su [[Category:Unbarred spiral galaxies]] ...

...used in [[astronomy]] to characterize the shape of [[spiral galaxy|spiral galaxies]].{{r|savres}} | title = Pitch angle variations in spiral galaxies ...

...from the study of [[planet]] [[atmosphere]]s to the evolution of [[Galaxy|galaxies]]. From 2010 until his death in late 2015 he was an [[emeritus]] professor ...rnal | author = Spinrad, H. | title = Stellar Populations in the Nuclei of Galaxies | journal = Publications of the Astronomical Society of the Pacific | volum ...

...Galaxies Catalogue|PGC]] 62756, [[Catalogue of Galaxies and of Clusters of Galaxies|CGCG]] 229-015, KIC 006932990, 2PBC J1905.3+4232}} [[Category:Ring galaxies]] ...

...p (also known as [[Lyons_Groups_of_Galaxies|LGG]] 33), which contains four galaxies, including [[NGC 701]] and [[IC 1738]].<ref>{{cite journal | bibcode=1993A& * [[List of spiral galaxies]] ...

...with black hole spins; for instance, [[relativistic jet|jets]] in [[active galaxies]] are believed to be launched parallel to the spin axes of supermassive bla ==Connection with radio galaxies== ...

=== 7. Rotational Speed of Galaxies === The theory offers a new way to describe the rotation of galaxies without the need for dark matter. The equation for the maximum rotation spe ...

...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 ...

...the understanding of early galaxy formation and the formation of low mass galaxies. He has since led major infrared surveys using ground-based telescopes suc ...utilises 180 orbits of the [[Hubble Space Telescope]] to image over 8000 [[galaxies]] in the near [[infrared]]. This is currently{{when|date=May 2016}} the lar ...

[[File:Analyzing Hot DOG Galaxies (PIA15815).jpg|thumb|Luminosity plot for hot DOGs and a prototypical [[lumi ...f their galactic mass in the central black hole than is observed in normal galaxies.<ref name="newsci20120830" /> ...

...ermassive black hole mass-Sérsic index relations for bulges and elliptical galaxies |journal=Monthly Notices of the Royal Astronomical Society |volume=434 |iss [[File:M33HunterWilson09.jpg|thumb|250px|Discs of spiral galaxies, such as the [[Triangulum Galaxy]], have low Sérsic indices and a low degre ...