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| Query : 2017ApJ...844...55Z |
2017ApJ...844...55Z - Astrophys. J., 844, 55-55 (2017/July-3)
Possible correlations between the emission properties of SGRBs and their offsets from the host galaxies.
ZHANG S., JIN Z.-P., ZHANG F.-W., LI X., FAN Y.-Z. and WEI D.-M.
Abstract (from CDS):
Short gamma-ray bursts (SGRBs) are widely believed to be from mergers of binary compact objects involving at least one neutron star and hence have a broad range of spatial offsets from their host galaxies. In this work, we search for possible correlations between the emission properties of 18 SGRBs and their offsets from the host galaxies. The SGRBs with and without extended emission do not show significant differences between their offset distributions, in agreement with some previous works. There are, however, possible correlations between the optical and X-ray afterglow emission and the offsets. The underlying physical origins are examined.
Abstract Copyright: © 2017. The American Astronomical Society. All rights reserved.
Journal keyword(s): gamma-ray burst: general - gamma rays: general - gamma rays: general
Simbad objects: 9
| Number of rows : 9 |
| 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 | Fermi bn100117879 | G | 00 45 04.6610 | -01 35 42.020 | ~ | 155 | 0 | |||||
| 2 | PSO J027.8085-18.5940 | G | 01 51 14.05011120 | -18 35 38.4976680 | ~ | 192 | 0 | |||||
| 3 | Fermi bn130925164 | gB | 02 44 42.38 | -26 09 15.8 | ~ | 184 | 0 | |||||
| 4 | SN 2006aj | SN* | 03 21 39.670 | +16 52 02.27 | 17.96 | 19.11 | 17.40 | SNIc-BL | 1007 | 1 | ||
| 5 | SDSS J112848.22+170418.5 | G | 11 28 48.22989 | +17 04 18.5014 | ~ | 393 | 0 | |||||
| 6 | GALEX J123205.0-105600 | Bz? | 12 32 04.9717245480 | -10 56 00.722548932 | 16.421 | ~ | 186 | 0 | ||||
| 7 | GRB 060614 | G | 21 23 32.140 | -53 01 36.10 | ~ | 714 | 0 | |||||
| 8 | GRB 061201 | gB | 22 08 32.060 | -74 34 47.90 | ~ | 205 | 0 | |||||
| 9 | NVSS J230126-385839 | rG | 23 01 26.7650 | -38 58 40.422 | 22.22 | 21.22 | 21 | ~ | 325 | 1 |
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