SwePub
Sök i LIBRIS databas

  Extended search

WFRF:(McCrum M.)
 

Search: WFRF:(McCrum M.) > (2010-2014) > INTERACTING SUPERNO...

INTERACTING SUPERNOVAE AND SUPERNOVA IMPOSTORS : SN 2009ip, IS THIS THE END?

Pastorello, A. (author)
Cappellaro, E. (author)
Inserra, C. (author)
show more...
Smartt, S. J. (author)
Pignata, G. (author)
Benetti, S. (author)
Valenti, S. (author)
Fraser, M. (author)
Takats, K. (author)
Benitez, S. (author)
Botticella, M. T. (author)
Brimacombe, J. (author)
Bufano, F. (author)
Cellier-Holzem, F. (author)
Costado, M. T. (author)
Cupani, G. (author)
Curtis, I. (author)
Elias-Rosa, N. (author)
Ergon, Mattias (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Fynbo, J. P. U. (author)
Hambsch, F. -J (author)
Hamuy, M. (author)
Harutyunyan, A. (author)
Ivarson, K. M. (author)
Kankare, E. (author)
Martin, J. C. (author)
Kotak, R. (author)
LaCluyze, A. P. (author)
Maguire, K. (author)
Mattila, S. (author)
Maza, J. (author)
McCrum, M. (author)
Miluzio, M. (author)
Norgaard-Nielsen, H. U. (author)
Nysewander, M. C. (author)
Ochner, P. (author)
Pan, Y. -C (author)
Pumo, M. L. (author)
Reichart, D. E. (author)
Tan, T. G. (author)
Taubenberger, S. (author)
Tomasella, L. (author)
Turatto, M. (author)
Wright, D. (author)
show less...
 (creator_code:org_t)
2013
2013
English.
In: Astrophysical Journal. - 0004-637X .- 1538-4357. ; 767:1, s. 1-
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • We report the results of a three-year-long dedicated monitoring campaign of a restless luminous blue variable (LBV) in NGC 7259. The object, named SN 2009ip, was observed photometrically and spectroscopically in the optical and near-infrared domains. We monitored a number of erupting episodes in the past few years, and increased the density of our observations during eruptive episodes. In this paper, we present the full historical data set from 2009 to 2012 with multi-wavelength dense coverage of the two high-luminosity events between 2012 August and September. We construct bolometric light curves and measure the total luminosities of these eruptive or explosive events. We label them the 2012a event (lasting similar to 50 days) with a peak of 3x10(41) erg s(-1), and the 2012b event (14 day rise time, still ongoing) with a peak of 8 x 1042 erg s(-1). The latter event reached an absolute R-band magnitude of about -18, comparable to that of a core-collapse supernova (SN). Our historical monitoring has detected high-velocity spectral features (similar to 13,000 km s(-1)) in 2011 September, one year before the current SN-like event. This implies that the detection of such high-velocity outflows cannot, conclusively, point to a core-collapse SN origin. We suggest that the initial peak in the 2012a event was unlikely to be due to a faint core-collapse SN. We propose that the high intrinsic luminosity of the latest peak, the variability history of SN 2009ip, and the detection of broad spectral lines indicative of high-velocity ejecta are consistent with a pulsational pair-instability event, and that the star may have survived the last outburst. The question of the survival of the LBV progenitor star and its future fate remain open issues, only to be answered with future monitoring of this historically unique explosion.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

galaxies: individual (NGC 7259)
supernovae: general
supernovae: individual (SN 2009ip
SN 2000ch)

Publication and Content Type

ref (subject category)
art (subject category)

Find in a library

To the university's database

Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.

 
pil uppåt Close

Copy and save the link in order to return to this view