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- Alicante_8 abstract "Alicante 8, also known as RSGC4, is a young massive open cluster belonging to the Milky Way galaxy. It was discovered in 2010 in the 2MASS survey data. As of 2010, the only members of the cluster that are currently identified are 8–13 red supergiants—young massive stars undergoing helium burning in their cores. The cluster is located in the constellation Scutum at the distance of about 20–23 kly (6–7 kpc) from the Sun. It is likely situated at the intersection of the northern end of the Long Bar of the Milky Way and the inner portion of the Scutum–Centaurus Arm—one of the two major spiral arms.The age of Alicante 8 is estimated at 16–20 million years. The observed red supergiants with the mass of about 12 solar masses are type II supernova progenitors. The cluster is heavily obscured and have not been detected in the visible light. It lies close to other groupings of red super giants known as RSGC1, Stephenson 2, and RSGC3. The mass of the open cluster is estimated at 10–20 thousand solar masses, which makes it one of the most massive open clusters in the Galaxy.".
- Alicante_8 wikiPageID "29595312".
- Alicante_8 wikiPageLength "2671".
- Alicante_8 wikiPageOutDegree "22".
- Alicante_8 wikiPageRevisionID "678451856".
- Alicante_8 wikiPageWikiLink 2MASS.
- Alicante_8 wikiPageWikiLink Bar.
- Alicante_8 wikiPageWikiLink Category:Open_clusters.
- Alicante_8 wikiPageWikiLink Category:Scutum_(constellation).
- Alicante_8 wikiPageWikiLink Category:Scutum–Centaurus_Arm.
- Alicante_8 wikiPageWikiLink Epoch_(astronomy).
- Alicante_8 wikiPageWikiLink Light.
- Alicante_8 wikiPageWikiLink Light-year.
- Alicante_8 wikiPageWikiLink Milky_Way.
- Alicante_8 wikiPageWikiLink Open_cluster.
- Alicante_8 wikiPageWikiLink Parsec.
- Alicante_8 wikiPageWikiLink RSGC1.
- Alicante_8 wikiPageWikiLink RSGC3.
- Alicante_8 wikiPageWikiLink Red_supergiant.
- Alicante_8 wikiPageWikiLink Scutum.
- Alicante_8 wikiPageWikiLink Scutum–Centaurus_Arm.
- Alicante_8 wikiPageWikiLink Solar_mass.
- Alicante_8 wikiPageWikiLink Stephenson_2.
- Alicante_8 wikiPageWikiLink Triple-alpha_process.
- Alicante_8 wikiPageWikiLink Type_II_supernova.
- Alicante_8 wikiPageWikiLink Year.
- Alicante_8 wikiPageWikiLinkText "Alicante 8".
- Alicante_8 age "16".
- Alicante_8 appmagV "not visible".
- Alicante_8 class "Open".
- Alicante_8 constellation Scutum.
- Alicante_8 distLy "~20 kly".
- Alicante_8 distPc "~6–7 kpc".
- Alicante_8 epoch Epoch_(astronomy).
- Alicante_8 massMsol "1".
- Alicante_8 name "Alicante 8".
- Alicante_8 names "RSGC4".
- Alicante_8 wikiPageUsesTemplate Template:Convert.
- Alicante_8 wikiPageUsesTemplate Template:DEC.
- Alicante_8 wikiPageUsesTemplate Template:E-sp.
- Alicante_8 wikiPageUsesTemplate Template:Infobox_open_cluster.
- Alicante_8 wikiPageUsesTemplate Template:RA.
- Alicante_8 wikiPageUsesTemplate Template:Reflist.
- Alicante_8 wikiPageUsesTemplate Template:Star-cluster-stub.
- Alicante_8 wikiPageUsesTemplate Template:Stellar_system.
- Alicante_8 subject Category:Open_clusters.
- Alicante_8 subject Category:Scutum_(constellation).
- Alicante_8 subject Category:Scutum–Centaurus_Arm.
- Alicante_8 hypernym Cluster.
- Alicante_8 type Language.
- Alicante_8 comment "Alicante 8, also known as RSGC4, is a young massive open cluster belonging to the Milky Way galaxy. It was discovered in 2010 in the 2MASS survey data. As of 2010, the only members of the cluster that are currently identified are 8–13 red supergiants—young massive stars undergoing helium burning in their cores. The cluster is located in the constellation Scutum at the distance of about 20–23 kly (6–7 kpc) from the Sun.".
- Alicante_8 label "Alicante 8".
- Alicante_8 sameAs Q4725676.
- Alicante_8 sameAs m.0fpjvw4.
- Alicante_8 sameAs Q4725676.
- Alicante_8 wasDerivedFrom Alicante_8?oldid=678451856.
- Alicante_8 isPrimaryTopicOf Alicante_8.