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- {{Short description|Open cluster in the constellation Coma Berenices}} {{Distinguish|Coma Cluster}} ...5 KB (721 words) - 02:44, 12 January 2025
- | name = α Persei |mark_link = α Persei ...17 KB (2,210 words) - 16:30, 8 June 2025
- {{Short description|Loose star cluster}} ...loose [[star cluster]], looser than both [[open cluster]]s and [[globular cluster]]s. Stellar associations will normally contain from 10 to 100 or more visib ...10 KB (1,399 words) - 00:39, 3 June 2025
- |genitive = Persei |brighteststarname = [[Alpha Persei|α Per]] (Mirfak) ...44 KB (6,245 words) - 15:35, 28 June 2025
- ...tars. The bright stars together are identified as the asterism [[Brocchi's Cluster|Coathanger]] resembling a [[Clothes hanger#The "Coathanger"|coathanger]], i ...the [[Taurus (constellation)|Taurus constellation]] and the [[Alpha Persei Cluster]] (with [[Alcyone (star)|Alcyone]] and [[Mirfak]] as the brightest stars). ...29 KB (4,188 words) - 19:42, 25 June 2025
- ...ral galaxy cores, [[Elliptical galaxy|elliptical galaxies]], or [[globular cluster]]s, most of which are believed to be composed of older stars, although the Many blue supergiant stars are [[Alpha Cygni variable|Alpha Cygni variables]].<ref name="Saio-2013">{{cite book|bibcode=2013ASPC..479.. ...21 KB (2,931 words) - 09:01, 10 June 2025
- | brighteststarname = [[Alpha Cassiopeiae|α Cas]] (Schedar){{efn|1=[[Gamma Cassiopeiae|γ Cas]] is variabl ...f the [[Milky Way]] runs through Cassiopeia, containing a number of [[open cluster]]s, young luminous galactic disc stars, and [[nebula]]e. [[IC 10]] is an ir ...41 KB (5,898 words) - 15:18, 28 June 2025
- ...located about {{convert|90,000|km}} from the planet.<ref>{{cite news|title=Cluster reveals the reformation of the Earth's bow shock|url=http://sci.esa.int/sci |[[Alpha Muscae]] ...18 KB (2,799 words) - 11:29, 25 March 2025
- ...l giant star can easily be larger than a hotter supergiant. For example, [[Alpha Herculis]] is classified as a giant star with a radius of {{solar radius|be ...=Maser mapping of small-scale structure in the circumstellar envelope of S Persei|journal=Monthly Notices of the Royal Astronomical Society|volume=306|issue= ...34 KB (4,945 words) - 21:26, 19 June 2025
- ...Tau group, including Epsilon Cassiopeiae, may have been separated from the cluster through tidal interactions.<ref name=aj117_1_354/> ...15 KB (1,953 words) - 20:16, 2 April 2025
- {{Short description|Binary star in the Pleiades star cluster}} | alt = Image of the Pleiades star cluster | float = center ...38 KB (5,347 words) - 14:45, 8 May 2025
- {{Short description|Type of star cluster}} {{Redirect-distinguish|Galactic cluster|galaxy cluster}} ...52 KB (7,643 words) - 23:47, 8 October 2025
- Its brightest star, [[Alpheratz]] (Alpha Andromedae), is a [[binary star]] that has also been counted as a part of [ .../startales/andromeda-alsufi.html|title=The Andromeda Galaxy and the Double Cluster in al-Sufi's Book of the Fixed Stars|publisher=Ian Ridpath's Star Tales |ac ...50 KB (6,601 words) - 00:29, 16 November 2025
- ...Jūn'', Great General of the Heaven)||[[γ Andromedae|γ And (Almach)]]||[[φ Persei|φ Per]]||[[51 Andromedae|51 And (Nembus)]]||[[49 Andromedae|49 And]]||[[χ A ...dromedae|62 And]]||HIP 10830||[[3 Persei|3 Per]]||[[2 Persei|2 Per]]||[[14 Persei|14 Per]]|| || || || || ...187 KB (19,494 words) - 18:42, 24 June 2025
- ...[[Milky Way|our galaxy]], astronomers have confirmed that no stars in that cluster exceed about {{nobr|150 {{Solar mass}}.}} ...2070 (captured by the Hubble Space Telescope).jpg|thumb|right|The [[R136]] cluster is an unusually dense collection of young, hot, blue stars.]] ...168 KB (21,234 words) - 12:04, 24 June 2025
- [[File:A Snapshot of the Jewel Box cluster with the ESO VLT.jpg|thumb|left|upright=1.0|The four brightest stars in [[N ...n be {{solar luminosity|over a million}} and are often unstable, such as [[Alpha Cygni variable|α Cygni variable]]s and [[luminous blue variable]]s. ...40 KB (5,846 words) - 10:33, 1 November 2025
- ...36.jpg|thumb|250px|A [[near-infrared]] image of the [[R136]] cluster. This cluster contains many of the most luminous known stars, including [[R136a1]]. ...osity|<var>L</var><sub>☉</sub>]] or greater, including the stars in [[open cluster]], [[OB association]] and [[H II region]]. The majority of stars thought to ...174 KB (22,432 words) - 19:46, 19 June 2025
- ...A || [[Alcyone (star)|Alcyone]] || Member of the [[Pleiades]] [[open star cluster]] ([[Messier objects|M45]]). [[Alcyone]] ({{langx|grc|Ἀλκυόνη}} {{translite ...literation|ar|al-jānib}} ('the flank'). Algenib is also another name for α Persei (Mirfak). ...109 KB (13,801 words) - 09:46, 27 June 2025
- ...roli]]''' ([[Latin (language)|Latin]] for 'heart of Charles') for the star Alpha Canum Venaticorum, so named in honour of [[King Charles I of England]] by S ...anev|'''Sualocin''' and '''Rotanev''']] for components of [[Alpha Delphini|Alpha]] and [[Beta Delphini]], two stars which appeared in the Palermo star catal ...43 KB (5,954 words) - 08:26, 24 May 2025
- ...its position near the winter [[Milky Way]], Auriga has many bright [[open cluster]]s in its borders, including [[Messier 36|M36]], [[Messier 37|M37]], and [[ ...a [[scimitar]] or crook. However, this may have represented just Capella (Alpha Aurigae) or the modern constellation as a whole; this figure was alternativ ...95 KB (13,211 words) - 15:15, 28 June 2025