The Ultraluminous X-Ray Sources Population of the Galaxy NGC 7456-Reference-Cited by-同舟云学术

The Ultraluminous X-Ray Sources Population of the Galaxy NGC 7456

Published:2020-02-26 Issue:2 Volume:890 Page:166
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Pintore F.,Marelli M.^ORCID,Salvaterra R.^ORCID,Israel G. L.^ORCID,Castillo G. A. Rodríguez,Esposito P.^ORCID,Belfiore A.^ORCID,Luca A. De,Wolter A.,Mereghetti S.^ORCID,Stella L.^ORCID,Rigoselli M.,Earnshaw H. P.^ORCID,Pinto C.,Roberts T. P.^ORCID,Walton D. J.^ORCID,Bernardini F.^ORCID,Haberl F.^ORCID,Salvaggio C.,Tiengo A.^ORCID,Zampieri L.^ORCID,Bachetti M.^ORCID,Brightman M.,Casella P.,D’Agostino D.^ORCID,Dall’Osso S.,Fürst F.^ORCID,Harrison F. A.,Mapelli M.^ORCID,Papitto A.^ORCID,Middleton M.^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/ab6ffd/pdf

Reference86 articles.

1. Observation of Gravitational Waves from a Binary Black Hole Merger

2. Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced Virgo

3. THE ULTRALUMINOUS X-RAY SOURCES NGC 1313 X-1 AND X-2: A BROADBAND STUDY WITHNuSTARANDXMM-Newton

4. In-depth studies of the NGC 253 ULXs withXMM-Newton: remarkable variability in ULX1, and evidence for extended coronae

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