A New Luminous Blue Variable in the Giant Extragalactic H [CSC]ii[/CSC] [CLC]Region NGC 2363[/CLC]
Open Access
- 1 January 1997
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 474 (1) , L35-L38
- https://doi.org/10.1086/310417
Abstract
We report the discovery of an erupting luminous blue variable (LBV) star in the giant H II region NGC 2363, the most massive star-forming region in the Magellanic irregular galaxy NGC 2366. This LBV, presently the visually brightest star in the galaxy (MV ~ -10.2), was first noticed in Hubble Space Telescope Wide Field Planetary Camera 2 images taken in 1996 January. An archival search allowed us to determine the onset of the present outburst. This star was not visible in 1991 nor 1992, but appeared in late 1993. In early 1995, it became the brightest star in the galaxy. The spectrum of the LBV displays a strong Hα emission line, as well as blueshifted absorption lines of He I.Keywords
This publication has 19 references indexed in Scilit:
- Was Fritz Zwicky's "Type V" SN 1961V a Genuine Supernova?The Astronomical Journal, 1995
- The Photometric Performance and Calibration of WFPC2Publications of the Astronomical Society of the Pacific, 1995
- The evolution of C/O in dwarf galaxies from Hubble Space Telescope FOS observationsThe Astrophysical Journal, 1995
- Violent star formation in NGC 2363The Astrophysical Journal, 1994
- The luminous blue variables: Astrophysical geysersPublications of the Astronomical Society of the Pacific, 1994
- A search for Wolf-Rayet stars in active star forming regions of low mass galaxies - GR8, NGC 2366, IC 2574, and NGC 1569The Astronomical Journal, 1993
- SN 1961V - an extragalactic ETA Carinae analogThe Astrophysical Journal, 1989
- The relation between apparent temperature and mass-loss rate in hypergiant eruptionsThe Astrophysical Journal, 1987
- Giant Outbursts of the Eta Carinae - P Cygni TypePublished by Springer Nature ,1987
- The Brightest Variable Stars in Extragalactic Nebulae. I. M31 and M33.The Astrophysical Journal, 1953