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| Query : 2002ApJ...575L..71V |
2002ApJ...575L..71V - Astrophys. J., 575, L71-L74 (2002/August-3)
LIGO/VIRGO searches for gravitational radiation in hypernovae.
VAN PUTTEN M.H.P.M.
Abstract (from CDS):
A torus around a stellar-mass Kerr black hole can emit about 10% of the spin energy of a black hole in gravitational radiation, which is potentially associated with a gamma-ray burst (GRB). Wide tori may develop buckling modes by the Papaloizou-Pringle instability and gravitational radiation-reaction forces in the Burke-Thorne approximation. Gravitational-wave experiments may discover these emissions in a fraction of nearby supernovae. This provides a test for Kerr black holes and for GRB inner engines by a comparison with the deredshifted durations of long GRBs.
Abstract Copyright: ∼
Journal keyword(s): Black Hole Physics - Gamma Rays: Bursts - Gamma Rays: Theory - Gravitational Waves
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 | GRB 000911 | gB | 02 18 42 | +07 48.0 | ~ | 163 | 0 | |||||
| 2 | GRB 011211 | gB | 11 15 16 | -21 56.0 | ~ | 305 | 0 | |||||
| 3 | GRB 011121 | gB | 11 34 26.67 | -76 01 41.6 | 23.0 | ~ | 286 | 1 | ||||
| 4 | V* V1033 Sco | HXB | 16 54 00.1423963019 | -39 50 44.761701340 | 16.14 | F3-6IV | 1980 | 0 | ||||
| 5 | V* V4641 Sgr | HXB | 18 19 21.6343259256 | -25 24 25.849595952 | 13.654 | 13.479 | 13.139 | B9III | 530 | 0 | ||
| 6 | SN 1998bw | SN* | 19 35 03.17 | -52 50 46.1 | 14.09 | SNIc | 1928 | 2 | ||||
| 7 | GRB 980703 | gB | 23 59 06.7 | +08 35 07 | ~ | 453 | 1 |
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