Electromagnetic counterparts of gravitational wave sources at the Very Large Telescope-Reference-Cited by-同舟云学术

Electromagnetic counterparts of gravitational wave sources at the Very Large Telescope

Published:2020-07-16 Issue:9 Volume:2 Page:455-457
ISSN:2522-5820
Container-title:Nature Reviews Physics
language:en
Short-container-title:Nat Rev Phys

Author:

Levan Andrew J.^ORCID,Jonker Peter G.^ORCID

Publisher

Springer Science and Business Media LLC

Subject

General Physics and Astronomy

Link

http://www.nature.com/articles/s42254-020-0216-2.pdf

Reference5 articles.

1. Mészáros, P. et al. Multi-messenger astrophysics. Nat. Rev. Phys. 1, 585–599 (2019).

2. Pian, E. et al. Spectroscopic identification of r-process nucleosynthesis in a double neutron-star merger. Nature 551, 67–70 (2017).

3. Smartt, S. J. et al. A kilonova as the electromagnetic counterpart to a gravitational-wave source. Nature 551, 75–79 (2017).

4. Covino, S. et al. The unpolarized macronova associated with the gravitational wave event GW 170817. Nat. Astron. 1, 791–794 (2017).

5. Ackley, K. et al. Observational constraints on the optical and near-infrared emission from the neutron star-black hole binary merger S190814bv. Preprint available at: arXiv: 2002.01950 (2020).

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