Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/44584
Title: No magnetars in ULXs
Authors: King, Andrew
Lasota, Jean-Pierre
First Published: 12-Mar-2019
Publisher: Oxford University Press (OUP), Royal Astronomical Society
Citation: Monthly Notices of the Royal Astronomical Society, 2019, 485 (3), pp. 3588-3594
Abstract: We consider the current observed ensemble of pulsing ultraluminous X-ray sources (PULXs). We show that all of their observed properties (luminosity, spin period, and spin-up rate) are consistent with emission from magnetic neutron stars with fields in the usual range 1011-1013 G, which is collimated ('beamed') by the outflow from an accretion disc supplied with mass at a super-Eddington rate, but ejecting the excess, in the way familiar for other (non-pulsing) ULXs. The observed properties are inconsistent with magnetar-strength fields in all cases. We point out that all proposed pictures of magnetar formation suggest that they are unlikely to be members of binary systems, in agreement with the observation that all confirmed magnetars are single. The presence of magnetars in ULXs is therefore improbable, in line with our conclusions above.
DOI Link: 10.1093/mnras/stz720
ISSN: 0035-8711
eISSN: 1365-2966
Links: https://academic.oup.com/mnras/article/485/3/3588/5376509
http://hdl.handle.net/2381/44584
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: Copyright © 2019, Oxford University Press (OUP), Royal Astronomical Society. Deposited with reference to the publisher’s open access archiving policy. (http://www.rioxx.net/licenses/all-rights-reserved)
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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