NGC 1579 explained

NGC 1579
Type:	H II region
Epoch:	J2000
Ra:	^[1]
Size V:	12' × 8'^[2]
Constellation:	Perseus^[3]
Radius Ly:	4
Names:	LBN 767, [B77] 70, Ced 35, LBN 165.38-08.73, [SS62] 19, DG 34, SH 2-222, [TP72] 12.

NGC 1579 (also known as the Northern Trifid) is a diffuse nebula located in the constellation of Perseus. It is referred to as the Northern Trifid because of its similar appearance to the Trifid Nebula, which is located in the southern celestial hemisphere of the sky. It is a H II region, a region of star formation.^[4]

The star cluster contains the emission-line star LkHα 101, which provides much of the ionizing radiation in the nebula.^[5]

NGC 1579 lies within a giant molecular cloud known as the California Molecular Cloud.^[6]

Notes and References

1. NGC 1579 . 2013-06-04.
2. Web site: Seligman. Courtney. Celestial Atlas: NGC Objects: NGC 1550 - 1599. cseligman.com. 11 July 2015. https://web.archive.org/web/20150315104558/http://cseligman.com/text/atlas/ngc15a.htm. live. 15 March 2015.
3. Web site: NGC 1579. Search results for NGC 1579. Wikisky. 5 June 2013.
4. Web site: A Hubble View of NGC 1579: The Trifid of the North . 7 Jun 2013 . 9 Jun 2013 .
5. LkHα 101 and the Young Cluster in NGC 1579. GH Herbig. 2004. Astronomical Journal. 128. 3. 1233–1253. 2004AJ....128.1233H. 10.1086/423043. 122724479 . free.
6. Lada. Charles J.. Lombardi. Marco. Alves. João. The California Molecular Cloud. 2009. Astronomical Journal. 703. 1. 52–59. 2009ApJ...703...52L. 10.1088/0004-637X/703/1/52. 0908.0646. 15371826 .