Swift Monitoring of M51: A 38 day Superorbital Period for the Pulsar ULX7 and a New Transient Ultraluminous X-Ray Source-Reference-Cited by-同舟云学术

Swift Monitoring of M51: A 38 day Superorbital Period for the Pulsar ULX7 and a New Transient Ultraluminous X-Ray Source

Published:2020-06-04 Issue:2 Volume:895 Page:127
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Brightman Murray,Earnshaw Hannah^ORCID,Fürst Felix^ORCID,Harrison Fiona A.,Heida Marianne^ORCID,Israel Gianluca^ORCID,Pike Sean^ORCID,Stern Daniel^ORCID,Walton Dominic J.^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/ab7e2a/pdf

Reference59 articles.

1. An ultraluminous X-ray source powered by an accreting neutron star

2. All at Once: Transient Pulsations, Spin-down, and a Glitch from the Pulsating Ultraluminous X-Ray Source M82 X-2

3. CHANDRA DETECTION OF SN 2010da FOUR MONTHS AFTER OUTBURST: EVIDENCE FOR A HIGH-MASS X-RAY BINARY IN NGC 300

4. Recurring X-ray outbursts in the supernova impostor SN 2010da in NGC 300

5. A Long Hard-X-Ray Look at the Dual Active Galactic Nuclei of M51 with NuSTAR

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3. A New Sample of Transient Ultraluminous X-Ray Sources Serendipitously Discovered by Swift/XRT;The Astrophysical Journal;2023-07-01

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