Gravitational-wave localization alone can probe origin of stellar-mass black hole mergers
Binary black hole mergers have recently been observed through the detection of gravitational wave signatures. The authors demonstrate that their association with active galactic nuclei can be made through a statistical spatial correlation.
Main Authors: | , , , , , |
---|---|
Format: | Article |
Language: | English |
Published: |
Nature Portfolio
2017-10-01
|
Series: | Nature Communications |
Online Access: | https://doi.org/10.1038/s41467-017-00851-7 |
_version_ | 1818750331306115072 |
---|---|
author | I. Bartos Z. Haiman Z. Marka B. D. Metzger N. C. Stone S. Marka |
author_facet | I. Bartos Z. Haiman Z. Marka B. D. Metzger N. C. Stone S. Marka |
author_sort | I. Bartos |
collection | DOAJ |
description | Binary black hole mergers have recently been observed through the detection of gravitational wave signatures. The authors demonstrate that their association with active galactic nuclei can be made through a statistical spatial correlation. |
first_indexed | 2024-12-18T04:17:58Z |
format | Article |
id | doaj.art-666c06326abd44e5b5c41457aa29a4ad |
institution | Directory Open Access Journal |
issn | 2041-1723 |
language | English |
last_indexed | 2024-12-18T04:17:58Z |
publishDate | 2017-10-01 |
publisher | Nature Portfolio |
record_format | Article |
series | Nature Communications |
spelling | doaj.art-666c06326abd44e5b5c41457aa29a4ad2022-12-21T21:21:17ZengNature PortfolioNature Communications2041-17232017-10-01811510.1038/s41467-017-00851-7Gravitational-wave localization alone can probe origin of stellar-mass black hole mergersI. Bartos0Z. Haiman1Z. Marka2B. D. Metzger3N. C. Stone4S. Marka5Columbia Astrophysics LaboratoryDepartment of Astronomy, Columbia UniversityColumbia Astrophysics LaboratoryColumbia Astrophysics LaboratoryColumbia Astrophysics LaboratoryColumbia Astrophysics LaboratoryBinary black hole mergers have recently been observed through the detection of gravitational wave signatures. The authors demonstrate that their association with active galactic nuclei can be made through a statistical spatial correlation.https://doi.org/10.1038/s41467-017-00851-7 |
spellingShingle | I. Bartos Z. Haiman Z. Marka B. D. Metzger N. C. Stone S. Marka Gravitational-wave localization alone can probe origin of stellar-mass black hole mergers Nature Communications |
title | Gravitational-wave localization alone can probe origin of stellar-mass black hole mergers |
title_full | Gravitational-wave localization alone can probe origin of stellar-mass black hole mergers |
title_fullStr | Gravitational-wave localization alone can probe origin of stellar-mass black hole mergers |
title_full_unstemmed | Gravitational-wave localization alone can probe origin of stellar-mass black hole mergers |
title_short | Gravitational-wave localization alone can probe origin of stellar-mass black hole mergers |
title_sort | gravitational wave localization alone can probe origin of stellar mass black hole mergers |
url | https://doi.org/10.1038/s41467-017-00851-7 |
work_keys_str_mv | AT ibartos gravitationalwavelocalizationalonecanprobeoriginofstellarmassblackholemergers AT zhaiman gravitationalwavelocalizationalonecanprobeoriginofstellarmassblackholemergers AT zmarka gravitationalwavelocalizationalonecanprobeoriginofstellarmassblackholemergers AT bdmetzger gravitationalwavelocalizationalonecanprobeoriginofstellarmassblackholemergers AT ncstone gravitationalwavelocalizationalonecanprobeoriginofstellarmassblackholemergers AT smarka gravitationalwavelocalizationalonecanprobeoriginofstellarmassblackholemergers |