Searching for propeller-phase ULXs in the XMM–Newton Serendipitous Source Catalogue
Author:
Affiliation:
1. Centre for Extragalactic Astronomy, Department of Physics, Durham University, South Road, Durham, DH1 3LE, UK
2. Cahill Center for Astronomy and Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA
Funder
Science and Technology Facilities Council
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/476/3/4272/24541947/sty501.pdf
Reference41 articles.
1. An ultraluminous X-ray source powered by an accreting neutron star
2. Testing the Paradigm that Ultraluminous X‐Ray Sources as a Class Represent Accreting Intermediate‐Mass Black Holes
3. SPECTRAL AND TEMPORAL PROPERTIES OF THE ULTRA-LUMINOUS X-RAY PULSAR IN M82 FROM 15 YEARS OFCHANDRAOBSERVATIONS AND ANALYSIS OF THE PULSED EMISSION USINGNuSTAR
4. THE FADING OF TWO TRANSIENT ULTRALUMINOUS X-RAY SOURCES TO BELOW THE STELLAR MASS EDDINGTON LIMIT
5. NuSTAR J095551+6940.8: a highly magnetized neutron star with super-Eddington mass accretion
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