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| Query : 2014ApJ...785...70D |
2014ApJ...785...70D - Astrophys. J., 785, 70 (2014/April-2)
Long gamma-ray bursts trace the star formation history.
DADO S. and DAR A.
Abstract (from CDS):
We show that if the broad-line supernova explosions of Type Ic (SNeIc) produce the bulk of the observed long duration gamma-ray bursts (LGRBs), including high- and low-luminosity LGRBs and X-ray flashes, and if the LGRBs have the geometry assumed in the cannonball model of LGRBs, then their rate, measured by Swift, and their redshift distribution are consistent with the star formation rate (SFR) over the entire range of redshifts where the SFR has been measured with sufficient accuracy.
Abstract Copyright: ∼
Journal keyword(s): gamma-ray burst: general - supernovae: general
Simbad objects: 7
| Number of rows : 7 |
| 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 | SN 2006aj | SN* | 03 21 39.670 | +16 52 02.27 | 17.96 | 19.11 | 17.40 | SNIc-BL | 1007 | 1 | ||
| 2 | SN 2010bh | SN* | 07 10 30.63 | -56 15 19.7 | SNIc | 336 | 1 | |||||
| 3 | SN 1998bw | SN* | 19 35 03.17 | -52 50 46.1 | 14.09 | SNIc | 1928 | 2 | ||||
| 4 | GRB 060614 | G | 21 23 32.140 | -53 01 36.10 | ~ | 714 | 0 | |||||
| 5 | GRB 060505 | gB | 22 07 03.440 | -27 48 51.89 | ~ | 286 | 1 | |||||
| 6 | GRB 020903 | gB | 22 48 42.34 | -20 46 09.3 | ~ | 248 | 1 | |||||
| 7 | GRB 051109B | gB | 23 01 50.330 | +38 40 46.51 | ~ | 93 | 0 |
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