A peculiarly short-duration gamma-ray burst from massive star core collapse-Reference-Cited by-同舟云学术

A peculiarly short-duration gamma-ray burst from massive star core collapse

Published:2021-07-26 Issue:9 Volume:5 Page:911-916
ISSN:2397-3366
Container-title:Nature Astronomy
language:en
Short-container-title:Nat Astron

Author:

Zhang B.-B.^ORCID,Liu Z.-K.,Peng Z.-K.,Li Y.,Lü H.-J.,Yang J.,Yang Y.-S.,Yang Y.-H.^ORCID,Meng Y.-Z.,Zou J.-H.,Ye H.-Y.^ORCID,Wang X.-G.,Mao J.-R.,Zhao X.-H.,Bai J.-M.,Castro-Tirado A. J.^ORCID,Hu Y.-D.,Dai Z.-G.,Liang E.-W.,Zhang B.^ORCID

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

https://www.nature.com/articles/s41550-021-01395-z.pdf

Reference43 articles.

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3. Abbott, B. P. et al. Multi-messenger observations of a binary neutron star merger. Astrophys. J. 848, L12–L70 (2017).

4. Zhang, B. et al. Discerning the physical origins of cosmological gamma-ray bursts based on multiple observational criteria: the cases of z = 6.7 GRB 080913, z = 8.2 GRB 090423, and some short/hard GRBs. Astrophys. J. 703, 1696–1724 (2009).

5. Gehrels, N. et al. A new γ-ray burst classification scheme from GRB 060614. Nature 444, 1044–1046 (2006).

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