NGC 4523 explained
NGC 4523 is a Magellanic spiral galaxy located about 35 to 50 million light-years away[3] in the constellation Coma Berenices.[4] It was discovered by astronomer Heinrich d'Arrest on April 19, 1865.[5] NGC 4523 is a member of the Virgo Cluster.[6] [7] A distance of (13 ± 2 Mpc) for NGC 4523 was derived from using yellow supergiants in the galaxy as standard candles.
On December 23, 1999, a Type II supernova designated as SN 1999gq was detected in NGC 4523.[8] [9]
See also
Notes and References
- Web site: NASA/IPAC Extragalactic Database . Results for NGC 4523 . 2017-12-04.
- Web site: parsecs to lightyears conversion. 2017-09-30.
- Web site: Your NED Search Results. ned.ipac.caltech.edu. 2017-12-04.
- Web site: Revised NGC Data for NGC 4523. spider.seds.org. 2017-12-04.
- Web site: New General Catalog Objects: NGC 4500 - 4549. cseligman.com. 2017-11-08.
- Shanks. T.. Tanvir. N. R.. Major. J. V.. Doel. A. P.. Dunlop. C. N.. Myers. R. M.. 1992-05-01. High-resolution imaging of Virgo cluster galaxies – II. Detection of the brightest stars in NGC 4523. Monthly Notices of the Royal Astronomical Society. en. 256. 1. 29P–32P. 10.1093/mnras/256.1.29p. 0035-8711. 1992MNRAS.256P..29S. free.
- Web site: The Virgo Cluster. www.atlasoftheuniverse.com. 2017-12-04.
- Web site: 1999gq - The Open Supernova Catalog. sne.space. en-US. 2017-12-05. 2017-12-06. https://web.archive.org/web/20171206074520/https://sne.space/sne/1999gq/. dead.
- Web site: Supernova 1999gq in NGC 4523. www.rochesterastronomy.org. 2017-12-05.