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- Q27994 subject Q6420423.
- Q27994 subject Q7009873.
- Q27994 subject Q7033717.
- Q27994 subject Q7152546.
- Q27994 subject Q7152550.
- Q27994 subject Q7216027.
- Q27994 subject Q8529982.
- Q27994 subject Q8606001.
- Q27994 subject Q8810647.
- Q27994 subject Q9125659.
- Q27994 abstract "IC 10 is an irregular galaxy in the constellation Cassiopeia. It was discovered by Lewis Swift in 1887. Nicholas Mayall was the first to suggest that the object is extragalactic in 1935. Edwin Hubble suspected it might belong to the Local Group of galaxies, but its status remained uncertain for decades. The radial velocity of IC 10 was measured in 1962, and it was found to be approaching the Milky Way at approximately350 km/s, strengthening the evidence for its membership in the Local Group. Its membership in the group was finally confirmed in 1996 by direct measurements of itsdistance based on observations of Cepheids. Despite its closeness, the galaxy is rather difficult to study because it lies near the plane of the Milky Way and is therefore heavily obscured by interstellar matter.The apparent distance between IC 10 and the Andromeda Galaxy is about the same as the apparent distance between the Andromeda Galaxy and the Triangulum Galaxy, which suggests that IC 10 may belong to the M31 subgroup.IC 10 is the only known starburst galaxy in the Local Group of galaxies. It has many more Wolf-Rayet stars per square kiloparsec (5.1 stars/kpc²) than the Large Magellanic Cloud (2.0 stars/kpc²) or the Small Magellanic Cloud (0.9 stars/kpc²). Although the galaxy has a luminosity similar to the SMC, it is considerably smaller. Its higher metallicity compared to the SMC suggests that star formation activity has continued for a longer time period. The evolutionary status of the Wolf-Rayet stars suggests that they all formed in a relatively short timespan. The ratio between the two types of Wolf-Rayet stars (WC stars and WN stars) in IC 10 is very different from the ratio in other galaxies in the Local Group, which may be somehow due to the starburst nature of the galaxy. Currently the galaxy produces stars at the rate of 0.04–0.08 solar masses per year, which means that the gas supply in the galaxy can last for only a few billion years longer.Observations of IC 10 in the far-infrared show that the dust in this mild starburst galaxy is deficient in small grains. It is hypothesized that any small grains that formerly existed were destroyed by strong ultraviolet radiation in the areas around the hot luminous stars that were formed in the galaxy's recent burst of star formation.The galaxy has a huge envelope of hydrogen gas, with an apparent size measuring 68′ × 80′, which is far larger than the apparent size of the galaxy in visible light (5.5′ × 7.0′). IC 10 is also unusual in the respect that the visible part of the galaxy seems to rotate in a different direction than the outer envelope. It has a H II nucleus.".
- Q27994 thumbnail IC10_BVHa.jpg?width=300.
- Q27994 wikiPageExternalLink i0010.html.
- Q27994 wikiPageExternalLink blackholeic10.htm.
- Q27994 wikiPageExternalLink IC10.html.
- Q27994 wikiPageWikiLink Q10464.
- Q27994 wikiPageWikiLink Q11282.
- Q27994 wikiPageWikiLink Q11391.
- Q27994 wikiPageWikiLink Q11574.
- Q27994 wikiPageWikiLink Q12129.
- Q27994 wikiPageWikiLink Q13724.
- Q27994 wikiPageWikiLink Q1479861.
- Q27994 wikiPageWikiLink Q180892.
- Q27994 wikiPageWikiLink Q188593.
- Q27994 wikiPageWikiLink Q190397.
- Q27994 wikiPageWikiLink Q193384.
- Q27994 wikiPageWikiLink Q217030.
- Q27994 wikiPageWikiLink Q240105.
- Q27994 wikiPageWikiLink Q2469.
- Q27994 wikiPageWikiLink Q2659211.
- Q27994 wikiPageWikiLink Q2703.
- Q27994 wikiPageWikiLink Q314284.
- Q27994 wikiPageWikiLink Q318.
- Q27994 wikiPageWikiLink Q321.
- Q27994 wikiPageWikiLink Q3944.
- Q27994 wikiPageWikiLink Q41872.
- Q27994 wikiPageWikiLink Q43027.
- Q27994 wikiPageWikiLink Q49957.
- Q27994 wikiPageWikiLink Q49984.
- Q27994 wikiPageWikiLink Q531.
- Q27994 wikiPageWikiLink Q5434654.
- Q27994 wikiPageWikiLink Q556.
- Q27994 wikiPageWikiLink Q615925.
- Q27994 wikiPageWikiLink Q6251.
- Q27994 wikiPageWikiLink Q6420423.
- Q27994 wikiPageWikiLink Q6472.
- Q27994 wikiPageWikiLink Q7009873.
- Q27994 wikiPageWikiLink Q7033717.
- Q27994 wikiPageWikiLink Q7152546.
- Q27994 wikiPageWikiLink Q7152550.
- Q27994 wikiPageWikiLink Q7216027.
- Q27994 wikiPageWikiLink Q726611.
- Q27994 wikiPageWikiLink Q8529982.
- Q27994 wikiPageWikiLink Q8606001.
- Q27994 wikiPageWikiLink Q8810647.
- Q27994 wikiPageWikiLink Q8928.
- Q27994 wikiPageWikiLink Q9125659.
- Q27994 name "IC 10".
- Q27994 names "UGC 192, PGC 1305".
- Q27994 type Place.
- Q27994 type CelestialBody.
- Q27994 type Galaxy.
- Q27994 type Location.
- Q27994 type Place.
- Q27994 type Thing.
- Q27994 type Q318.
- Q27994 comment "IC 10 is an irregular galaxy in the constellation Cassiopeia. It was discovered by Lewis Swift in 1887. Nicholas Mayall was the first to suggest that the object is extragalactic in 1935. Edwin Hubble suspected it might belong to the Local Group of galaxies, but its status remained uncertain for decades. The radial velocity of IC 10 was measured in 1962, and it was found to be approaching the Milky Way at approximately350 km/s, strengthening the evidence for its membership in the Local Group.".
- Q27994 label "IC 10".
- Q27994 depiction IC10_BVHa.jpg.
- Q27994 name "IC 10".
- Q27994 name "UGC192,PGC1305".
