| dc.contributor.author | Melandri, A. | |
| dc.contributor.author | D'Elia, V | |
| dc.contributor.author | Campana, S. | |
| dc.contributor.author | D'Ai, A. | |
| dc.contributor.author | Emery, S. W. K. | |
| dc.contributor.author | Frederiks, D. D. | |
| dc.contributor.author | Lien, A. | |
| dc.contributor.author | Page, K. L. | |
| dc.contributor.author | Starling, R. L. C. | |
| dc.contributor.author | Burrows, D. N. | |
| dc.contributor.author | Breeveld, A. A. | |
| dc.contributor.author | Oates, S. R. | |
| dc.contributor.author | O'Brien, P. T. | |
| dc.contributor.author | Osborne, J. P. | |
| dc.contributor.author | Siegel, M. H. | |
| dc.contributor.author | Tagliaferri, G. | |
| dc.contributor.author | Brown, P. J. | |
| dc.contributor.author | Cenko, S. B. | |
| dc.contributor.author | Svinkin, D. S. | |
| dc.contributor.author | Tohuvavohu, A. | |
| dc.contributor.author | Tsvetkova, A. E. | |
| dc.contributor.author | De Pasquale, M. | |
| dc.date.accessioned | 2021-03-03T19:13:59Z | |
| dc.date.available | 2021-03-03T19:13:59Z | |
| dc.identifier.citation | D'Elia V., Campana S., D'Ai A., De Pasquale M., Emery S. W. K. , Frederiks D. D. , Lien A., Melandri A., Page K. L. , Starling R. L. C. , et al., "GRB 171205A/SN2017iuk: A local low-luminosity gamma-ray burst", ASTRONOMY & ASTROPHYSICS, cilt.619, 2018 | |
| dc.identifier.issn | 1432-0746 | |
| dc.identifier.other | vv_1032021 | |
| dc.identifier.other | av_53748794-109e-4fa4-9f6a-856d8d5b6047 | |
| dc.identifier.uri | http://hdl.handle.net/20.500.12627/59162 | |
| dc.identifier.uri | https://doi.org/10.1051/0004-6361/201833847 | |
| dc.description.abstract | Context. Gamma-ray bursts (GRBs) occurring in the local Universe constitute an interesting sub-class of the GRB family, since their luminosity is on average lower than that of their cosmological analogs. Attempts to understand in a global way this peculiar behaviour is still not possible, since the sample of low redshift GRBs is small, and the properties of individual objects are too different from each other. In addition, their closeness (and consequently high fluxes) make these sources ideal targets for extensive follow-up even with small telescopes, considering also that these GRBs are conclusively associated with supernova (SN) explosions. | |
| dc.language.iso | eng | |
| dc.subject | Temel Bilimler (SCI) | |
| dc.subject | ASTRONOMİ VE ASTROFİZİK | |
| dc.subject | Uzay bilimi | |
| dc.subject | Fizik | |
| dc.subject | Astronomi ve Astrofizik | |
| dc.subject | Temel Bilimler | |
| dc.title | GRB 171205A/SN2017iuk: A local low-luminosity gamma-ray burst | |
| dc.type | Makale | |
| dc.relation.journal | ASTRONOMY & ASTROPHYSICS | |
| dc.contributor.department | Italian Space Agency , , | |
| dc.identifier.volume | 619 | |
| dc.contributor.firstauthorID | 103724 | |
