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Query : 2014MNRAS.443...67M |
2014MNRAS.443...67M - Mon. Not. R. Astron. Soc., 443, 67-71 (2014/September-1)
An upper limit to the energy of gamma-ray bursts indicates that GRBs/SNe are powered by magnetars.
MAZZALI P.A., McFADYEN A.I., WOOSLEY S.E., PIAN E. and TANAKA M.
Abstract (from CDS):
Abstract Copyright: © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2014)
Journal keyword(s): gamma-ray burst: general - stars: magnetars - supernovae: general
Simbad objects: 14
Number of rows : 14 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | GRB 000911 | gB | 02 18 42 | +07 48.0 | ~ | 156 | 0 | |||||
2 | SN 2006aj | SN* | 03 21 39.670 | +16 52 02.27 | 17.96 | 19.11 | 17.40 | SNIc-BL | 940 | 1 | ||
3 | M 1 | SNR | 05 34 30.9 | +22 00 53 | ~ | 6197 | 1 | |||||
4 | SN 2010bh | SN* | 07 10 30.63 | -56 15 19.7 | SNIc | 287 | 1 | |||||
5 | SN 2003lw | SN* | 08 02 30.1 | -39 51 03 | 20.23 | SNIc: | 548 | 0 | ||||
6 | SN 2012bz | SN* | 09 07 38.38 | +14 01 07.5 | SNIb/c | 163 | 1 | |||||
7 | GRB 111211A | gB | 10 12 21.700 | +11 12 30.00 | ~ | 33 | 0 | |||||
8 | SN 2005bf | SN* | 10 23 56.99 | -03 11 29.3 | 18.0 | SNIb | 204 | 1 | ||||
9 | SN 2003dh | SN* | 10 44 50.030 | +21 31 18.15 | 16.2 | SNIcpec | 1209 | 1 | ||||
10 | SN 2013cq | SN* | 11 32 32.84 | +27 41 56.2 | SNIc | 516 | 1 | |||||
11 | SN 2010ah | SN* | 11 44 02.99 | +55 41 27.6 | SNIc | 51 | 1 | |||||
12 | SN 2013dx | SN* | 14 29 14.77 | +15 46 26.6 | ~ | 151 | 0 | |||||
13 | GRB 080319B | gB | 14 31 41.04 | +36 18 09.2 | ~ | 467 | 0 | |||||
14 | SN 1998bw | SN* | 19 35 03.17 | -52 50 46.1 | 14.09 | SNIc | 1825 | 2 |
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