SwePub
Sök i LIBRIS databas

  Extended search

(WFRF:(Anderson Kevin)) srt2:(2010-2014)
 

Search: (WFRF:(Anderson Kevin)) srt2:(2010-2014) > SN 2009bb :

SN 2009bb : A PECULIAR BROAD-LINED TYPE Ic SUPERNOVA

Pignata, Giuliano (author)
Stritzinger, Maximilian (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Soderberg, Alicia (author)
show more...
Mazzali, Paolo (author)
Phillips, M. M. (author)
Morrell, Nidia (author)
Anderson, J. P. (author)
Boldt, Luis (author)
Campillay, Abdo (author)
Contreras, Carlos (author)
Folatelli, Gaston (author)
Foerster, Francisco (author)
Gonzalez, Sergio (author)
Hamuy, Mario (author)
Krzeminski, Wojtek (author)
Maza, Jose (author)
Roth, Miguel (author)
Salgado, Francisco (author)
Levesque, Emily M. (author)
Rest, Armin (author)
Crain, J. Adam (author)
Foster, Andrew C. (author)
Haislip, Joshua B. (author)
Ivarsen, Kevin M. (author)
LaCluyze, Aaron P. (author)
Nysewander, Melissa C. (author)
Reichart, Daniel E. (author)
show less...
 (creator_code:org_t)
2011
2011
English.
In: Astrophysical Journal. - 0004-637X .- 1538-4357. ; 728:1, s. 14-
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • Ultraviolet, optical, and near-infrared photometry and optical spectroscopy of the broad-lined Type Ic supernova (SN) 2009bb are presented, following the flux evolution from -10 to +285 days past B-band maximum. Thanks to the very early discovery, it is possible to place tight constraints on the SN explosion epoch. The expansion velocities measured from near maximum spectra are found to be only slightly smaller than those measured from spectra of the prototype broad-lined SN 1998bw associated with GRB 980425. Fitting an analytical model to the pseudobolometric light curve of SN 2009bb suggests that 4.1 +/- 1.9M(circle dot) of material was ejected with 0.22 +/- 0.06 M(circle dot) of it being (56)Ni. The resulting kinetic energy is 1.8 +/- 0.7 x 10(52) erg. This, together with an absolute peak magnitude of M(B) = -18.36 +/- 0.44, places SN 2009bb on the energetic and luminous end of the broad-lined Type Ic (SN Ic) sequence. Detection of helium in the early time optical spectra accompanied with strong radio emission and high metallicity of its environment makes SN 2009bb a peculiar object. Similar to the case for gamma-ray bursts (GRBs), we find that the bulk explosion parameters of SN 2009bb cannot account for the copious energy coupled to relativistic ejecta, and conclude that another energy reservoir (a central engine) is required to power the radio emission. Nevertheless, the analysis of the SN 2009bb nebular spectrum suggests that the failed GRB detection is not imputable to a large angle between the line-of-sight and the GRB beamed radiation. Therefore, if a GRB was produced during the SN 2009bb explosion, it was below the threshold of the current generation of gamma-ray instruments.

Subject headings

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

Keyword

galaxies: individual (NGC 3278)
supernovae: general
supernovae: individual (SN 2009bb)

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