SN2010U -- a Luminous Nova in NGC 4214
arXiv:1005.4356 · doi:10.1088/2041-8205/718/1/L43
Abstract
The luminosity, light curve, post--maximum spectrum, and lack of a progenitor on deep pre-outburst images suggest that SN 2010U was a luminous, fast nova. Its outburst magnitude is consistent with that for a fast nova using the Maximum Magnitude-Rate of Decline relationship for classical novae.
8 pages, 4 figures
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Cited by in corpus (7)
- Luminous Blue Variable eruptions and related transients: Diversity of progenitors and outburst properties
- Discovery of Precursor LBV Outbursts in Two Recent Optical Transients: The Fitfully Variable Missing Links UGC 2773-OT and SN 2009ip
- Supernovae and their host galaxies. I. The SDSS DR8 database and statistics
- A unified supernova catalogue
- The Chandra Local Volume Survey I: The X-ray Point Source Populations of NGC 55, NGC 2403, and NGC 4214
- The ACS Nearby Galaxy Survey Treasury VII. The NGC 4214 Starburst and the Effects of Star Formation History on Dwarf Morphology
- The Unusually Luminous Extragalactic Nova SN 2010U