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Interacting supernovae and supernova impostors. SN 2007sv: the major eruption of a massive star in UGC 5979
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2015 (English)In: Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, E-ISSN 1365-2966, Vol. 447, no 1, 117-131 p.Article in journal (Refereed) Published
Abstract [en]

We report the results of the photometric and spectroscopic monitoring campaign of the transient SN 2007sv. The observables are similar to those of Type IIn supernovae, a well-known class of objects whose ejecta interact with pre-existing circumstellar material (CSM). The spectra show a blue continuum at early phases and prominent Balmer lines in emission; however, the absolute magnitude at the discovery of SN 2007sv (M-R=-14.25 +/- 0.38) indicate it to be most likely a supernova impostor. This classification is also supported by the lack of evidence in the spectra of very high velocity material as expected in supernova ejecta. In addition, we find no unequivocal evidence of broad lines of alpha- and/or Fe-peak elements. The comparison with the absolute light curves of other interacting objects (including Type IIn supernovae) highlights the overall similarity with the prototypical impostor SN 1997bs. This supports our claim that SN 2007sv was not a genuine supernova, and was instead a supernova impostor, most likely similar to the major eruption of a luminous blue variable.

Place, publisher, year, edition, pages
2015. Vol. 447, no 1, 117-131 p.
Keyword [en]
supernovae: individual: SN 2007sv, galaxies: individual: UGC 5979
National Category
Astronomy, Astrophysics and Cosmology
URN: urn:nbn:se:su:diva-115924DOI: 10.1093/mnras/stu2384ISI: 000350272700008OAI: diva2:805987


Available from: 2015-04-17 Created: 2015-04-08 Last updated: 2015-04-17Bibliographically approved

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Taddia, Francesco
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Department of AstronomyThe Oskar Klein Centre for Cosmo Particle Physics (OKC)
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