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arXiv:0710.5173 (astro-ph)
[Submitted on 26 Oct 2007]

Title:The Broad-lined Type Ic SN 2003jd

Authors:S. Valenti, S. Benetti, E. Cappellaro, F. Patat, P. Mazzali, M. Turatto, K. Hurley, K. Maeda, A. Gal-Yam, R. J. Foley, A. V. Filippenko, A. Pastorello, P. Challis, F. Frontera, A. Harutyunyan, M. Iye, K. Kawabata, R. P. Kirshner, W. Li, Y. M. Lipkin, T. Matheson, K. Nomoto, E. O. Ofek, Y. Ohyama, E. Pian, M. Salvo, D. N. Sauer, B. P. Schmidt, A. Soderberg, L. Zampieri
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Abstract: The results of a world-wide coordinated observational campaign on the broad-lined Type Ic SN 2003jd are presented. In total, 74 photometric data points and 26 spectra were collected using 11 different telescopes. SN 2003jd is one of the most luminous SN Ic ever observed. A comparison with other Type Ic supernovae (SNe Ic) confirms that SN 2003jd represents an intermediate case between broad-line events (2002ap, 2006aj), and highly energetic SNe (1997ef, 1998bw, 2003dh, 2003lw), with an ejected mass of M_{ej} = 3.0 +/- 1 Mo and a kinetic energy of E_{k}(tot) = 7_{-2}^{+3} 10^{51} erg. SN 2003jd is similar to SN 1998bw in terms of overall luminosity, but it is closer to SNe 2006aj and 2002ap in terms of light-curve shape and spectral evolution. The comparison with other SNe Ic, suggests that the V-band light curves of SNe Ic can be partially homogenized by introducing a time stretch factor. Finally, due to the similarity of SN 2003jd to the SN 2006aj/XRF 060218 event, we discuss the possible connection of SN 2003jd with a GRB.
Comments: 19 pages, 19 figures, Accepted for publication in MNRAS
Subjects: Astrophysics (astro-ph)
Cite as: arXiv:0710.5173 [astro-ph]
  (or arXiv:0710.5173v1 [astro-ph] for this version)
  https://doi.org/10.48550/arXiv.0710.5173
Related DOI: https://doi.org/10.1111/j.1365-2966.2007.12647.x

Submission history

From: Stefano Valenti [view email]
[v1] Fri, 26 Oct 2007 20:04:50 UTC (753 KB)
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