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The broad-lined type Ic supernova 2003jd

delete2007-12-17
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OA
AI
V
Valenti, S. *
B
Benetti, S.
C
Cappellaro, E.
P
Patat, F.
M
Mazzali, P.
T
Turatto, M.
H
Hurley, K.
M
Maeda, K.
G
Gal-Yam, A.
F
Foley, R. J.
F
Filippenko, A. V.
P
Pastorello, A.
C
Challis, P.
F
Frontera, F.
H
Harutyunyan, A.
I
Iye, M.
K
Kawabata, K.
K
Kirshner, R. P.
L
Li, W.
L
Lipkin, Y. M.
M
Matheson, T.
N
Nomoto, K.
O
Ofek, E. O.
O
Ohyama, Y.
P
Pian, E.
P
Poznanski, D.
S
Salvo, M.
S
Sauer, D. N.
S
Schmidt, B. P.
S
Soderberg, A.
Z
Zampieri, L.
DOI:10.1111/j.1365-2966.2007.12647.xdelete
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摘要

摘要

En 中文
The results of a worldwide coordinated observational campaign on the broad-lined Type Ic supernova (SN Ic) 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 +/- 1M(circle dot) and a kinetic energy of Ek(tot)=7(-2)(+3) x 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, because of the similarity of SN 2003jd to the SN 2006aj/XRF 060218 event, we discuss the possible connection of SN 2003jd with a gamma-ray burst (GRB).
Keyword:
supernovae : general
supernovae : individual
2003jd
supernovae : individual : 1996aq
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Monthly Notices of the Royal Astronomical Society 封面图
Monthly Notices of the Royal Astronomical Society
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California Institute of Technology
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University of Tokyo
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national institutes of natural sciences (nins) - japan
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Harvard University
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University of Ferrara
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University of Padua
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Smithsonian Institution
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University of California System
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Tel Aviv University
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national astronomical observatory of japan (naoj)
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istituto nazionale astrofisica (inaf)
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引用论文

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Hydrogen in type Ic supernovae?
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SN 1994I: Disentangling He I lines in Type Ic supernovae
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errClocchiatti, A; Wheeler, JC; Brotherton, MS; Cochran, AL; Wills, D; Barker, ES; Turatto, M
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The metamorphosis of SN 1998bw
err2001-07-10
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errPatat, F; Cappellaro, E; Danziger, J; Mazzali, PA; Sollerman, J; Augusteijn, T; Brewer, J; Doublier, V; Gonzalez, JF; Hainaut, O; Lidman, C; Leibundgut, B; Nomoto, K; Nakamura, T; Spyromilio, J; Rizzi, L; Turatto, M; Walsh, J; Galama, TJ; van Paradijs, J; Kouveliotou, C; Vreeswijk, PM; Frontera, F; Masetti, N; Palazzi, E; Pian, E
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