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- Q16933736 subject Q10638.
- Q16933736 subject Q8432416.
- Q16933736 subject Q9107096.
- Q16933736 subject Q9168518.
- Q16933736 abstract "SDSS J1229+1122 (SDSS J122952.66+112227.8) is a blue supergiant O-type star in the tail of dwarf irregular galaxy IC 3418. It illuminates a nebula clump of gas, and was discovered from the spectrum of the illumination source. The clump of gas resides in a tail caused by ram pressure stripping of gas from the galaxy by the galaxy cluster. It was determined to be a blue supergiant through analysis of its spectrum. As of 2013, it is the most distant known star, at 55×10^6 ly (17 Mpc) (stars more distant than this are only known through events that they cause, such as stellar explosions of supernovae and gamma ray bursts). The discovery was made by Drs. Youichi Ohyama and Ananda Hota, using the Subaru Telescope. The star and its galaxy is in the Virgo Cluster of galaxies. The clump of gas that the star illuminates is referred to as D3 or IC3418 D3, and lies within a filamentary structure referred to as F1 or IC3418 F1. The galactic tail and all within it are escaping the galaxy to become intracluster flotsam, unattached to any galaxy, just the cluster.".
- Q16933736 wikiPageWikiLink Q1048372.
- Q16933736 wikiPageWikiLink Q10638.
- Q16933736 wikiPageWikiLink Q190397.
- Q16933736 wikiPageWikiLink Q22247.
- Q16933736 wikiPageWikiLink Q2703.
- Q16933736 wikiPageWikiLink Q271818.
- Q16933736 wikiPageWikiLink Q3686787.
- Q16933736 wikiPageWikiLink Q3937.
- Q16933736 wikiPageWikiLink Q42372.
- Q16933736 wikiPageWikiLink Q840332.
- Q16933736 wikiPageWikiLink Q841079.
- Q16933736 wikiPageWikiLink Q8432416.
- Q16933736 wikiPageWikiLink Q8842.
- Q16933736 wikiPageWikiLink Q9107096.
- Q16933736 wikiPageWikiLink Q9168518.
- Q16933736 type Place.
- Q16933736 type CelestialBody.
- Q16933736 type Location.
- Q16933736 type Place.
- Q16933736 type Star.
- Q16933736 type Thing.
- Q16933736 comment "SDSS J1229+1122 (SDSS J122952.66+112227.8) is a blue supergiant O-type star in the tail of dwarf irregular galaxy IC 3418. It illuminates a nebula clump of gas, and was discovered from the spectrum of the illumination source. The clump of gas resides in a tail caused by ram pressure stripping of gas from the galaxy by the galaxy cluster. It was determined to be a blue supergiant through analysis of its spectrum.".
- Q16933736 label "SDSS J1229+1122".