The analogy of K-correction in the topic of gamma-ray bursts
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F19%3A10408849" target="_blank" >RIV/00216208:11320/19:10408849 - isvavai.cz</a>
Výsledek na webu
<a href="https://doi.org/10.1017/S1743921318008025" target="_blank" >https://doi.org/10.1017/S1743921318008025</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1017/S1743921318008025" target="_blank" >10.1017/S1743921318008025</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
The analogy of K-correction in the topic of gamma-ray bursts
Popis výsledku v původním jazyce
It is well-known that there are two types of gamma-ray bursts (GRBs): short/hard and long/soft ones, respectively. The long GRBs are coupled to supernovae, but the short ones are associated with the so called macronovae (also known as kilonovae), which can serve as the sources of gravitational waves as well. The kilonovae can arise from the merging of two neutron-stars. The neutron stars can be substituded by more massive black holes as well. Hence, the topic of gamma-ray bursts (mainly the topic of short ones) and the topic of massive binaries, are strongly connected.In this contribution, the redshifts of GRBs are studied. The surprising result - namely that the apparently fainter GRBs can be in average at smaller distances - is discussed again. In essence, the results of Mészáros et al. (2011) are studied again using newer samples of GRBs. The former result is confirmed by the newer data. (C) International Astronomical Union 2019.
Název v anglickém jazyce
The analogy of K-correction in the topic of gamma-ray bursts
Popis výsledku anglicky
It is well-known that there are two types of gamma-ray bursts (GRBs): short/hard and long/soft ones, respectively. The long GRBs are coupled to supernovae, but the short ones are associated with the so called macronovae (also known as kilonovae), which can serve as the sources of gravitational waves as well. The kilonovae can arise from the merging of two neutron-stars. The neutron stars can be substituded by more massive black holes as well. Hence, the topic of gamma-ray bursts (mainly the topic of short ones) and the topic of massive binaries, are strongly connected.In this contribution, the redshifts of GRBs are studied. The surprising result - namely that the apparently fainter GRBs can be in average at smaller distances - is discussed again. In essence, the results of Mészáros et al. (2011) are studied again using newer samples of GRBs. The former result is confirmed by the newer data. (C) International Astronomical Union 2019.
Klasifikace
Druh
D - Stať ve sborníku
CEP obor
—
OECD FORD obor
10308 - Astronomy (including astrophysics,space science)
Návaznosti výsledku
Projekt
—
Návaznosti
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Ostatní
Rok uplatnění
2019
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název statě ve sborníku
Proceedings of the International Astronomical Union
ISBN
—
ISSN
1743-9213
e-ISSN
1743-9221
Počet stran výsledku
3
Strana od-do
380-382
Název nakladatele
Cambridge University Press
Místo vydání
UK
Místo konání akce
Vienna, Austria
Datum konání akce
27. 8. 2018
Typ akce podle státní příslušnosti
WRD - Celosvětová akce
Kód UT WoS článku
—