Log in to save to my catalogue

Properties and astrophysical implications of the 150 Msun binary black hole merger GW190521

Properties and astrophysical implications of the 150 Msun binary black hole merger GW190521

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2439764063

Properties and astrophysical implications of the 150 Msun binary black hole merger GW190521

About this item

Full title

Properties and astrophysical implications of the 150 Msun binary black hole merger GW190521

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2020-09

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

The gravitational-wave signal GW190521 is consistent with a binary black hole merger source at redshift 0.8 with unusually high component masses, \(85^{+21}_{-14}\,M_{\odot}\) and \(66^{+17}_{-18}\,M_{\odot}\), compared to previously reported events, and shows mild evidence for spin-induced orbital precession. The primary falls in the mass gap pred...

Alternative Titles

Full title

Properties and astrophysical implications of the 150 Msun binary black hole merger GW190521

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2439764063

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2439764063

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.2009.01190

How to access this item