2008ApJ...687L...9M


Query : 2008ApJ...687L...9M

2008ApJ...687L...9M - Astrophys. J., 687, L9-L12 (2008/November-1)

Double-peaked oxygen lines are not rare in nebular spectra of core-collapse supernovae.

MODJAZ M., KIRSHNER R.P., BLONDIN S., CHALLIS P. and MATHESON T.

Abstract (from CDS):

Double-peaked oxygen lines in the nebular spectra of two peculiar Type Ib/c supernovae (SNe Ib/c) have been interpreted as off-axis views of a GRB jet or unipolar blob ejections. Here we present late-time spectra of eight SNe IIb, Ib, and Ic and show that this phenomenon is common and should not be so firmly linked to extraordinary explosion physics. The line profiles are most likely caused by ejecta expanding with a torus- or disk-like geometry. Double-peaked oxygen profiles are not necessarily the indicator of a misdirected GRB jet.

Abstract Copyright: ∼

Journal keyword(s): Gamma Rays: Bursts - Stars: Supernovae: General

Simbad objects: 18

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Number of rows : 18
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 12317 1
2 SNR B0102-72.3 SNR 01 04 01.2 -72 01 52           ~ 422 1
3 SN 2004gv SN* 02 13 37.42 -00 43 05.8     17.6     SNIb 47 1
4 SN 1984L SN* 02 35 30.54 -07 09 30.3   14.0       SNIb 197 1
5 SN 2006aj SN* 03 21 39.670 +16 52 02.27 17.96 19.11 17.40     SNIc-BL 1007 1
6 SN 1996N SN* 03 38 55.37 -26 20 04.0       16   SNIb 49 2
7 SN 2004gq SN* 05 12 04.81 -15 40 54.2     15.5     SNIb 105 1
8 SN 1987A SN* 05 35 27.98840 -69 16 11.1134           SNIIpec 5203 2
9 SN 2006T SN* 09 54 30.21 -25 42 29.3     17.2     SNIIb 67 1
10 SN 2005bf SN* 10 23 56.99 -03 11 29.3     18.0     SNIb 225 1
11 SN 2004gt SN* 12 01 50.37 -18 52 12.7   19.42 14.9     SNIc 86 1
12 SN 2004gk SN* 12 25 33.21 +12 15 39.9     13.3     SNIc 46 1
13 SN 1990I SN* 12 44 50.26 -40 43 36.5   16.7 16.7     SNIb 62 1
14 SN 1994I SN* 13 29 54.072 +47 11 30.50     12.9     SNIc 645 1
15 SN 1983N SN* 13 36 51.23 -29 54 01.7   11.7       SNIb 278 1
16 SN 2004dk SN* 16 21 48.93 -02 16 17.3   17.789 17.6     SNIb 98 1
17 SN 2004ao SN* 17 28 09.35 +07 24 55.5     14.9     SNIb 49 1
18 SN 2003jd SN* 23 21 03.38 -04 53 45.5   16.34       SNIc-BL 147 1

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