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Probing the nature of the low state in the extreme ultraluminous X-ray pulsar NGC 5907 ULX1

Fürst, F.; Walton, D. J.; Israel, G. L.; Bachetti, M.; Barret, D.; Brightman, M.; Earnshaw, H. P.; Fabian, A.; Heida, M.; Imbrogno, M.; Middleton, M. J.; Pinto, C.; Salvaterra, R.; Roberts, T. P.; Rodríguez Castillo, G. A.; Webb, N.

Probing the nature of the low state in the extreme ultraluminous X-ray pulsar NGC 5907 ULX1 Thumbnail


Authors

F. Fürst

D. J. Walton

G. L. Israel

M. Bachetti

D. Barret

M. Brightman

H. P. Earnshaw

A. Fabian

M. Heida

M. Imbrogno

M. J. Middleton

C. Pinto

R. Salvaterra

G. A. Rodríguez Castillo

N. Webb



Abstract

NGC 5907 ULX1 is the most luminous ultra-luminous X-ray pulsar (ULXP) known to date, reaching luminosities in excess of 1041 erg s−1. The pulsar is known for its fast spin-up during the on-state. Here, we present a long-term monitoring of the X-ray flux and the pulse period between 2003 and 2022. We find that the source was in an off- or low-state between mid-2017 to mid-2020. During this state, our pulse period monitoring shows that the source had spun down considerably. We interpret this spin-down as likely being due to the propeller effect, whereby accretion onto the neutron star surface is inhibited. Using state-of-the-art accretion and torque models, we use the spin-up and spin-down episodes to constrain the magnetic field. For the spin-up episode, we find solutions for magnetic field strengths of either around 1012 G or 1013 G, however, the strong spin-down during the off-state seems only to be consistent with a very high magnetic field, namely, > 1013 G. This is the first time a strong spin-down is seen during a low flux state in a ULXP. Based on the assumption that the source entered the propeller regime, this gives us the best estimate so far for the magnetic field of NGC 5907 ULX1.

Citation

Fürst, F., Walton, D. J., Israel, G. L., Bachetti, M., Barret, D., Brightman, M., …Webb, N. (2023). Probing the nature of the low state in the extreme ultraluminous X-ray pulsar NGC 5907 ULX1. Astronomy & Astrophysics, 672, Article A140. https://doi.org/10.1051/0004-6361/202245048

Journal Article Type Article
Acceptance Date Jan 23, 2023
Online Publication Date Apr 12, 2023
Publication Date 2023-04
Deposit Date Nov 8, 2023
Publicly Available Date Nov 8, 2023
Journal Astronomy & Astrophysics
Print ISSN 0004-6361
Electronic ISSN 1432-0746
Publisher EDP Sciences
Peer Reviewed Peer Reviewed
Volume 672
Article Number A140
DOI https://doi.org/10.1051/0004-6361/202245048
Keywords Space and Planetary Science; Astronomy and Astrophysics
Public URL https://durham-repository.worktribe.com/output/1901923

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Copyright Statement
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. This article is published in open access under the Subscribe to Open model. Subscribe to A&A to support open access publication.




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