No magnetars in ULXs
- 12 March 2019
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 485 (3) , 3588-3594
Abstract
No abstract availableKeywords
All Related Versions
Funding Information
- National Science Centre (2015/19/B/ST9/01099)
This publication has 68 references indexed in Scilit:
- The supergiant optical counterpart of ULX P13 in NGC 7793Astronomische Nachrichten, 2011
- Ultraluminous X-ray sources out toz~ 0.3 in the COSMOS fieldAstronomy & Astrophysics, 2010
- Masses, beaming and Eddington ratios in ultraluminous X-ray sourcesMonthly Notices of the Royal Astronomical Society: Letters, 2009
- XMM-Newton discovery of transient X-ray pulsar in NGC 1313Monthly Notices of the Royal Astronomical Society: Letters, 2008
- ChandraandXMM‐NewtonDiscovery of Transient X‐Ray Pulsar in the Nearby Spiral Galaxy NGC 2403The Astrophysical Journal, 2007
- Supercritically accreting stellar mass black holes as ultraluminous X-ray sourcesMonthly Notices of the Royal Astronomical Society, 2007
- The nature of SS433 and the ultraluminous X-ray sourcesMonthly Notices of the Royal Astronomical Society, 2006
- A Variable Ultraluminous Supersoft X‐Ray Source in “The Antennae”: Stellar‐Mass Black Hole or White Dwarf?The Astrophysical Journal, 2003
- Ultraluminous X-Ray Sources in External GalaxiesThe Astrophysical Journal, 2001
- The Nature of Accreting Black Holes in Nearby Galaxy NucleiThe Astrophysical Journal, 1999