2007PASP..119.1211F


C.D.S. - SIMBAD4 rel 1.7 - 2020.03.29CET01:46:55

2007PASP..119.1211F - Publ. Astron. Soc. Pac., 119, 1211-1232 (2007/November-0)

Constraints on type Ib/c supernovae and gamma-ray burst progenitors.

FRYER C.L., MAZZALI P.A., PROCHASKA J., CAPPELLARO E., PANAITESCU A., BERGER E., VAN PUTTEN M., VAN DEN HEUVEL E.P.J., YOUNG P., HUNGERFORD A., ROCKEFELLER G., YOON S.-C., PODSIADLOWSKI P., NOMOTO K., CHEVALIER R., SCHMIDT B. and KULKARNI S.

Abstract (from CDS):

Although there is strong support for the collapsar engine as the power source of long-duration gamma-ray bursts (GRBs), we still do not definitively know the progenitor of these explosions. Here we review the current set of progenitor scenarios for long-duration GRBs and the observational constraints on these scenarios. Examining these models, we find that single stars cannot be the only progenitor for long-duration GRBs. Several binary progenitors can match the solid observational constraints and also have the potential to match the trends that we are currently seeing in the observations. Type Ib/c supernovae are also likely to be produced primarily in binaries; we discuss the relationship between the progenitors of these explosions and those of the long-duration GRBs.

Abstract Copyright:

Journal keyword(s): Reviews

Status at CDS:  

Simbad objects: 27

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Number of rows : 27

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 GRB 021004 gB 00 26 54.68 +18 55 41.6           ~ 511 1
2 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 9278 1
3 SN 2002ap SN* 01 36 23.85 +15 45 13.2   13.11 14.54     SNIc-BL 487 1
4 SN 2006aj SN* 03 21 39.670 +16 52 02.27 17.96 19.11 17.40     SNIc-BL 817 1
5 GRB 991216 gB 05 09 31.2983 +11 17 07.262           ~ 404 1
6 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 14610 1
7 SN 1987A SN* 05 35 28.020 -69 16 11.07   4.75 4.81     SNIIpec 4430 2
8 SN 1997ef SN* 07 57 02.87 +49 33 41.3     16.5     SNIc-BL 247 1
9 SN 2003lw SN* 08 02 30.1 -39 51 03       20.23   SNIc: 501 0
10 SN 1993J SN* 09 55 24.77476 +69 01 13.7026   10.8 12.0     SNIIb 1239 1
11 NGC 3125 H2G 10 06 33.318 -29 56 07.32 13.03 13.45 13.00 12.50 13.4 ~ 213 1
12 SN 2003dh SN* 10 44 50.030 +21 31 18.15     16.2     SNIcpec 1103 2
13 GRB 011211 gB 11 15 16 -21 56.0           ~ 284 1
14 GRB 030226 gB 11 33 04.9 +25 53 56           ~ 185 2
15 V* BP Cru HXB 12 26 37.5607088371 -62 46 13.259605389   12.70 10.66     B1.5Iaeq 597 0
16 SN 1994I SN* 13 29 54.072 +47 11 30.50     12.9     SNIc 562 1
17 GRB 990510 gB 13 38 07.64 -80 29 48.8           ~ 463 1
18 GRB 010222 gB 14 52 12.55 +43 01 06.3           ~ 334 2
19 GRB 990123 gB 15 25 29 +44 45.0     8.95     ~ 960 1
20 GRB 000301C gB 16 20 18.5 +29 26 35           ~ 339 2
21 GRB 000926 gB 17 04 15 +51 46.0           ~ 340 2
22 SN 1998bw SN* 19 35 03.17 -52 50 46.1   14.09       SNIc 1632 2
23 GRB 020813A gB 19 46 41.874 -19 36 04.81           ~ 282 1
24 HD 226868 HXB 19 58 21.6758193269 +35 12 05.782512305 9.38 9.72 8.91 8.42   O9.7Iabpvar 3888 0
25 SN 2001ig SN* 22 57 30.69 -41 02 25.9     14.5     SNIIb 138 1
26 GRB 980519 gB 23 22 21.5 +77 15 43           ~ 193 0
27 NAME Cas A SNR 23 23 24.000 +58 48 54.00           ~ 2375 1

    Equat.    Gal    SGal    Ecl

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2020.03.29-01:46:55

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