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Gamma-ray bursts: A brief survey of the diversity

Published online by Cambridge University Press:  30 December 2019

Attila Mészáros Open the ORCID record for Attila Mészáros [Opens in a new window]  and
Jakub Řípa Open the ORCID record for Jakub Řípa [Opens in a new window]
Attila Mészáros
Affiliation:
Astronomical Institute, Faculty of Mathematics and Physics, Charles University, CZ-180 00 Prague 8, V Holešovičkách 2, Czech Republic email: [email protected]
Jakub Řípa
Affiliation:
Astronomical Institute, Faculty of Mathematics and Physics, Charles University, CZ-180 00 Prague 8, V Holešovičkách 2, Czech Republic email: [email protected] MTA-Eötvös Lóránd University, Lendület Hot Universe Research Group, Pázmány Péter sétány 1/A, Budapest, 1117, Hungary Eötvös Lóránd University, Institute of Physics, Pázmány Péter sétány 1/A, Budapest, 1117, Hungary email: [email protected]
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Abstract

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The separation of the gamma-ray bursts (GRBs) into short/hard and long/soft subclasses, respectively, is well supported both theoretically and observationally. The long ones are coupled to supernovae type Ib/Ic - the short ones are connected to the merging of two neutron stars, where one or even both neutron stars can be substituted by black holes. These short GRBs - as merging binaries - can also serve as the sources of gravitation waves, and are observable as the recently detected macronovae. Since 1998 there are several statistical studies suggesting the existence of more than two subgroups. There can be a subgroup having an intermediate durations; there can be a subgroup with ultra-long durations; the long/soft subgroup itself can be divided into two subclasses with respect to the luminosity of GRBs. The authors with other collaborators provided several statistical studies in this topic. This field of the GRB-diversity is briefly surveyed in this contribution.

Keywords

cosmology: miscellaneouscosmology: observationsgamma rays: bursts
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S346: High-mass X-ray Binaries: Illuminating the Passage from Massive Binaries to Merging Compact Objects , August 2018 , pp. 383 - 387
Copyright
© International Astronomical Union 2019 

References

Abbott, B. P., et al. 2017, ApJ (Letters), 848, L13 Google Scholar
Acuner, Z., & Ryde, F. 2018, MNRAS, 475, 1708 CrossRefGoogle Scholar
Colgate, S. A. 1968, Canadian Journal of Physics (Supplement), 46, 476 CrossRefGoogle Scholar
Colgate, S. A. 1974, ApJ, 187, 333 CrossRefGoogle Scholar
Fenimore, E. E., et al. 1995, ApJ (Letters), 448, L101 Google Scholar
Gehrels, N., et al. 2006, Nature, 444, 1044 CrossRefGoogle Scholar
Hjorth, J., et al. 2003, Nature. 423, 847 CrossRefGoogle Scholar
Hakkila, J., et al. 2003, ApJ, 582, 320 CrossRefGoogle Scholar
Hakkila, J., et al. 2004, Baltic Astronomy, 13, 2011 Google Scholar
Horváth, I. 1998, ApJ, 508, 757 CrossRefGoogle Scholar
Horváth, I. 2002, A&A, 392, 791 Google Scholar
Horváth, I., et al. 2006, A&A, 447, 23 Google Scholar
Kann, D. A., et al. 2010, ApJ, 720, 1513 CrossRefGoogle Scholar
Kass, R. E., & Raftery, A. E. 1995, Journal of the American Statistical Association, 90, 773 CrossRefGoogle Scholar
Klebesadel, R. W., Strong, I. B., & Olson, R. A. 1974, ApJ (Letters), 182, L85 Google Scholar
Levan, A. J., Tanvir, N. R., & Starling, R. L. C. 2014, ApJ, 781, 13 CrossRefGoogle Scholar
Mazets, E. P., et al. 1981, ApSS, 80, 3 Google Scholar
Mészáros, A., & Mészáros, P. 1996, ApJ, 466, 29 CrossRefGoogle Scholar
Mészáros, P. 2006, Reports on Progress in Physics, 69, 2259 CrossRefGoogle Scholar
Mukherjee, S., et al. 1998, ApJ, 508, 314 CrossRefGoogle Scholar
Narayana Bhat, P., et al. 2016, ApJ (Suppl.), 223, id.28 CrossRefGoogle Scholar
Ohmori, N., et al. 2016, PASJ, 68, S30 CrossRefGoogle Scholar
Pendleton, G. N., et al. 1997, ApJ, 489, 175 CrossRefGoogle Scholar
Řípa, J., et al. 2012, ApJ, 756, id.44 CrossRefGoogle Scholar
Řípa, J., & Mészáros, A. 2016, ApSS, 361, id.370 Google Scholar
Ruffini, R., et al. 2018, ApJ, 859, id.30 CrossRefGoogle Scholar
Tanvir, N. R., et al. 2013, Nature, 500, 547 CrossRefGoogle Scholar
Tarnopolski, M. 2015 A&A, 581, id.A29 Google Scholar
Tarnopolski, M. 2016, MNRAS, 458, 2024 CrossRefGoogle Scholar
Tikhomirova, Ya. Yu., & Stern, B. E. 2005, AstL, 31, 291 Google Scholar
Tsvetkova, A., et al. 2017, ApJ, 850, id.161 CrossRefGoogle Scholar
Veres, P., et al. 2010, ApJ, 725, 1955 CrossRefGoogle Scholar
Virgili, F. J., et al. 2015, ApJ, 778, id.54 CrossRefGoogle Scholar