Published July 2005
| Version v1
Journal article
SN/GRB connection: a statistical approach with BATSE and Asiago Catalogues
Creators
- 1. INAF Astronomical Observatory of Capodimonte, Napoli (Italy)
- 2. Ferrara Univ., Ferrara (Italy). Physics Department
- 3. INAF Astronomical Observatory of Arcetri, Florence (Italy)
- 4. INFN-IASF, Bologna (Italy)
- 5. Liverpool JM Univ., Birkenhead (United Kingdom). Astrophysic Research Institute
Description
Recent observations suggest that some types of GRB are physically connected with SNe of type Ib/c. However, it has been pointed out by several authors that some GRBs could be associated also with other types of core-collapse SNe (type Ildw/IIn). On the basis of a comprehensive statistical study, which has made use of the BATSE and Asiago catalogues, we have found that: i) the temporal and spatial distribution of SNe-Ib/c is marginally correlated with that of the BATSE GRBs; ii) we do not confirm the existence of an association between GRBs and SNe-IIdw/IIn
Availability note (English)
Also avalaible from: http://dx.doi.org/10.1393/ncc/i2005-10118-1Additional details
Identifiers
Publishing Information
- Journal Title
- Nuovo Cimento della Societa Italiana di Fisica. C, Geophysics and Space Physics
- Journal Volume
- 28C
- Journal Issue
- 4-5
- Journal Page Range
- p. 633-636
- ISSN
- 1124-1896
INIS
- Country of Publication
- Italy
- Country of Input or Organization
- Italy
- INIS RN
- 37047497
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Descriptors DEI
- COSMIC GAMMA BURSTS; COSMIC GAMMA SOURCES; GAMMA DETECTION; STATISTICS; SUPERNOVAE
- Descriptors DEC
- BINARY STARS; COSMIC RADIATION; COSMIC RAY SOURCES; DETECTION; ERUPTIVE VARIABLE STARS; IONIZING RADIATIONS; MATHEMATICS; PRIMARY COSMIC RADIATION; RADIATION DETECTION; RADIATIONS; STARS; VARIABLE STARS