About: Binary black hole merger rates inferred from luminosity function of ultra-luminous X-ray sources

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scholarly article by Yoshiyuki Inoue et al published 8 July 2016 in Monthly Notices of the Royal Astronomical Society

Attributes	Values
rdf:type	Item
description	wetenschappelijk artikel (nl) наукова стаття, опублікована в липні 2016 (uk) im Juli 2016 veröffentlichter wissenschaftlicher Artikel (de) scholarly article by Yoshiyuki Inoue et al published 8 July 2016 in Monthly Notices of the Royal Astronomical Society (en)
publication date	wds:Q58907512-AFDCB324-97FD-46AC-B16F-3C29A1562290
publication date	2016-07-08 00:00:00Z (xsd:dateTime)
language of work or name	wds:Q58907512-B328C8C1-7E1E-4CE1-8E4F-AB201E6D80EC
language of work or name	English
cites work	wds:Q58907512-0F66C1F3-53AA-40FF-92B7-5EB0456E44FC wds:Q58907512-152DE8F0-2D39-47A1-ADCF-09847A73DF98 wds:Q58907512-184033AD-C528-4AFA-B24D-EFFE3D84532E wds:Q58907512-1B06F44C-D023-4093-870D-BA2C51DF5DDD wds:Q58907512-2A9B6010-1A97-40FF-B7B5-3AC512F1AAD5 wds:Q58907512-32922918-B0A5-43AF-AB09-CD81D55ADE21 wds:Q58907512-45012B0B-2A34-4003-B41A-DAAEF37DDFE5 wds:Q58907512-5E3358EB-1733-47F4-8CA3-7F5305A7141A wds:Q58907512-677D1344-24FB-4AC6-B957-88D180F33E6F wds:Q58907512-6E498729-B85D-488D-A53F-F11F14BB3C3F wds:Q58907512-711B3068-DAB5-4E16-A6D6-B6B241C8F4E3 wds:Q58907512-A9AA151C-BD7F-4269-B58E-8CABB0EC8F99 wds:Q58907512-ADBD1860-0D53-49AE-B260-F0CAEC2AD5FD wds:Q58907512-B336331B-51B9-490F-93F5-EA5103736CDA wds:Q58907512-BF1DB5E8-16E3-41E1-B740-F18B9CC5F19F wds:Q58907512-C0E0E3F7-BB0B-4314-ADB9-949F83BCF0ED wds:Q58907512-C2E71DF9-2AA5-482C-A0BE-2F79FB6CF235 wds:Q58907512-CBBFF660-C8CA-43CB-B88D-83BBFA678179 wds:Q58907512-D7F9126D-C3A0-4386-BC5A-47B1AADAE405 wds:Q58907512-E3658BD2-C6B4-48A4-954A-182D3C46202B wds:Q58907512-F0D40CEB-9472-4878-BE86-CCD549B29F0E wds:Q58907512-FCB9B9F6-D442-4721-80BF-7F640E29BE8B
cites work	The Ultraluminous X‐Ray Source Population from theChandraArchive of Galaxies A new test of general relativity - Gravitational radiation and the binary pulsar PSR 1913+16 Observation of Gravitational Waves from a Binary Black Hole Merger Astrophysical Implications of the Binary Black-hole Merger GW150914 Discovery of a pulsar in a binary system The first gravitational-wave source from the isolated evolution of two stars in the 40-100 solar mass range GW150914: The Advanced LIGO Detectors in the Era of First Discoveries Merging binary black holes formed through chemically homogeneous evolution in short-period stellar binaries Binary interaction dominates the evolution of massive stars. Advanced Virgo: a second-generation interferometric gravitational wave detector Gravitational Radiation and the Motion of Two Point Masses The Evolution of Compact Binary Star Systems Binary Black Hole Mergers from Globular Clusters: Implications for Advanced LIGO. Characterization of the LIGO detectors during their sixth science run Fermi GBM observations of LIGO gravitational-wave event GW150914 An ultraluminous X-ray source powered by an accreting neutron star Binary Mergers and Growth of Black Holes in Dense Star Clusters Dynamical interactions and the black-hole merger rate of the Universe Extragalactic background light from hierarchical galaxy formation: gamma-ray attenuation up to the epoch of cosmic reionization and the first stars Puzzling accretion onto a black hole in the ultraluminous X-ray source M 101 ULX-1. A mass of less than 15 solar masses for the black hole in an ultraluminous X-ray source The Total Merger Rate of Compact Object Binaries in the Local Universe
author name string	wds:Q58907512-0550BD46-F731-43FF-8346-CE14F69E5C58 wds:Q58907512-5B7F69AE-BC0D-4ADF-B9D7-9979DB380A13
author name string	Naoki Isobe Yasuyuki T. Tanaka
rdfs:label	Binary black hole merger rates inferred from luminosity function of ultra-luminous X-ray sources (en) Binary black hole merger rates inferred from luminosity function of ultra-luminous X-ray sources (nl)
skos:prefLabel	Binary black hole merger rates inferred from luminosity function of ultra-luminous X-ray sources (en) Binary black hole merger rates inferred from luminosity function of ultra-luminous X-ray sources (nl)
name	Binary black hole merger rates inferred from luminosity function of ultra-luminous X-ray sources (en) Binary black hole merger rates inferred from luminosity function of ultra-luminous X-ray sources (nl)
author	wds:Q58907512-86BF818D-8064-4412-BD9B-F2C057D4DA68
author	Yoshiyuki Inoue
title	wds:Q58907512-B7A8F03C-AA64-49AA-9DDB-25D4FE732412
title	Binary black hole merger rates inferred from luminosity function of ultra-luminous X-ray sources (en)
page(s)	wds:Q58907512-1FA560E2-B106-41DD-A349-6E1E39696716
page(s)	4329–4334
Internet Archive ID	wds:Q58907512-47BAAC44-42BA-47B6-91CA-ABD0E7934337
Internet Archive ID	arxiv-1602.05554
instance of	wds:Q58907512-1DC42BF9-9D46-4CDD-A7E0-B5D3CA7923FA
instance of	scholarly article
main subject	wds:Q58907512-8EA25C03-D532-41E6-BBE3-C0BD90873968
main subject	black hole
published in	wds:Q58907512-7154426D-F2D8-4B40-8387-695244FAA9D1
published in	Monthly Notices of the Royal Astronomical Society
issue	wds:Q58907512-9389DE48-6F80-4AF7-811C-69351B9B924F
volume	wds:Q58907512-1C26CC14-4AF7-4EE0-B8F3-8CC03FF0313D
issue	4
volume	461
number of pages	wds:Q58907512-871F3A9E-04FA-4193-9CD9-D0FE8B960353
number of pages	6 (xsd:decimal)
DOI	wds:Q58907512-77DB73CA-6062-4851-971D-6040D7C521A7
DOI	http://dx.doi.org/10.1093/MNRAS/STW1637
DOI	10.1093/MNRAS/STW1637
arXiv ID	wds:Q58907512-F27CB58C-D174-4FA0-A391-D0D366DD4230
arXiv ID	1602.05554
ADS bibcode	wds:Q58907512-64B65994-7102-4289-B730-258EE5878738
ADS bibcode	2016MNRAS.461.4329I
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q58907512

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