Published in
Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 2(433), p. 1312-1337
DOI: 10.1093/mnras/stt813
Links
- ORCID
- ORCID
- ORCID
- ORCID
- ORCID
- Oxford University Press (OUP) | PDF
- [arxiv.org] | PDF
- [www.researchgate.net] | PDF
- [citeseerx.ist.psu.edu] | PDF
- [www.mpa-garching.mpg.de] | PDF
- [pure.qub.ac.uk] | PDF
- [pure.qub.ac.uk] | PDF
- [arxiv.org] | PDF
Tools
SN 2009ip á la PESSTO: No evidence for core-collapse yet
,
Cosimo Inserra,
Anders Jerkstrand,
Rubina Kotak ,
Giuliano Pignata,
Stefano Benetti,
Maria-Teresa Botticella ,
Filomena Bufano,
Michael Childress,
Seppo Mattila,
Andrea Pastorello,
Stephen J. Smartt,
Massimo Turatto,
Fang Yuan,
Joe P. Anderson
and other authors.
Full text: Download
Abstract
We present observations of the interacting transient SN 2009ip, from the start of the outburst in October 2012 until the end of the 2012 observing season. The transient reached a peak of $M_V$=-17.7 mag before fading rapidly, with a total integrated luminosity of 1.9$\times10^{49}$ erg over the period of August-December 2012. The optical and near infrared spectra are dominated by narrow emission lines, signaling a dense circumstellar environment, together with multiple components of broad emission and absorption in H and He at velocities between 0.5-1.2$\times10^4$ km s$^{-1}$̇ We see no evidence for nucleosynthesized material in SN 2009ip, even in late-time pseudo-nebular spectra. We set a limit of $