Evidence for Low Kick Velocities among High-mass X-Ray Binaries in the Small Magellanic Cloud from the Spatial Correlation Function-Reference-Cited by-同舟云学术

Evidence for Low Kick Velocities among High-mass X-Ray Binaries in the Small Magellanic Cloud from the Spatial Correlation Function

Published:2021-09-28 Issue:2 Volume:919 Page:81
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Bodaghee Arash^ORCID,Antoniou Vallia^ORCID,Zezas Andreas^ORCID,Tomsick John A.^ORCID,Jordan Zachary,Jackson Brenton,Agnew Ryan,Frechette Eric,Hornschemeier Ann E.,Rodriguez Jérôme^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/ac11f4/pdf

Reference56 articles.

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3. THECHANDRASURVEY OF THE SMALL MAGELLANIC CLOUD “BAR”. II. OPTICAL COUNTERPARTS OF X-RAY SOURCES

4. EXPLORING THE OVERABUNDANCE OF ULXs IN METAL- AND DUST-POOR LOCAL LYMAN BREAK ANALOGS

5. The Most Ordinary Formation of the Most Unusual Double Black Hole Merger

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