The X-ray bursts of XTE J1739–285: a NICER sample
The X-ray bursts of XTE J1739–285: a NICER sample
In this work, we report on observations with the Neutron Star Interior Composition Explorer of the known neutron star X-ray transient XTE J1739-285. We observed the source in 2020 February and March, finding it in a highly active bursting state. Across a 20 day period, we detected 32 thermonuclear X-ray bursts, with an average burst recurrence time of 2.0-0.3+0.4 hr. A timing and spectral analysis of the ensemble of X-ray bursts reveals homogeneous burst properties, evidence for short-recurrence time bursts, and the detection of a 386.5 Hz burst oscillation candidate. The latter is especially notable, given that a previous study of this source claimed a 1122 Hz burst oscillation candidate. We did not find any evidence of variability near 1122 Hz and instead find that the 386.5 Hz oscillation is the more prominent signal of the two burst oscillation candidates. Hence, we conclude it is unlikely that XTE J1739-285 has a submillisecond rotation period.
1-12
Bult, Peter
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Altamirano, Diego
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Arzoumanian, Zaven
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Bilous, Anna V.
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Chakrabarty, Deepto
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Gendreau, Keith C.
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Güver, Tolga
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Jaisawal, Gaurava K.
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Kuulkers, Erik
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Malacaria, Christian
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Ng, Mason
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Sanna, Andrea
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Strohmayer, Tod E.
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1 February 2021
Bult, Peter
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Altamirano, Diego
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Arzoumanian, Zaven
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Bilous, Anna V.
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Chakrabarty, Deepto
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Gendreau, Keith C.
289c5283-377f-476a-aec3-5532dfff6f2b
Güver, Tolga
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Jaisawal, Gaurava K.
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Kuulkers, Erik
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Malacaria, Christian
309a8f91-28a7-4365-b0a3-633171fc2e51
Ng, Mason
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Sanna, Andrea
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Strohmayer, Tod E.
e1a6de84-d23d-43de-b33e-2d49c4a5daa7
Bult, Peter, Altamirano, Diego, Arzoumanian, Zaven, Bilous, Anna V., Chakrabarty, Deepto, Gendreau, Keith C., Güver, Tolga, Jaisawal, Gaurava K., Kuulkers, Erik, Malacaria, Christian, Ng, Mason, Sanna, Andrea and Strohmayer, Tod E.
(2021)
The X-ray bursts of XTE J1739–285: a NICER sample.
The Astrophysical Journal, 907 (2), , [79].
(doi:10.3847/1538-4357/abd54b).
Abstract
In this work, we report on observations with the Neutron Star Interior Composition Explorer of the known neutron star X-ray transient XTE J1739-285. We observed the source in 2020 February and March, finding it in a highly active bursting state. Across a 20 day period, we detected 32 thermonuclear X-ray bursts, with an average burst recurrence time of 2.0-0.3+0.4 hr. A timing and spectral analysis of the ensemble of X-ray bursts reveals homogeneous burst properties, evidence for short-recurrence time bursts, and the detection of a 386.5 Hz burst oscillation candidate. The latter is especially notable, given that a previous study of this source claimed a 1122 Hz burst oscillation candidate. We did not find any evidence of variability near 1122 Hz and instead find that the 386.5 Hz oscillation is the more prominent signal of the two burst oscillation candidates. Hence, we conclude it is unlikely that XTE J1739-285 has a submillisecond rotation period.
Text
The X-Ray Bursts of XTE J1739-285 A NICER Sample
- Accepted Manuscript
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Accepted/In Press date: 17 December 2020
Published date: 1 February 2021
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© 2021. The American Astronomical Society. All rights reserved..
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Local EPrints ID: 447831
URI: http://eprints.soton.ac.uk/id/eprint/447831
ISSN: 0004-637X
PURE UUID: 6806dc99-5c15-4a5a-a490-7c008b0e7d46
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Date deposited: 23 Mar 2021 17:40
Last modified: 12 Nov 2024 05:02
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Contributors
Author:
Peter Bult
Author:
Zaven Arzoumanian
Author:
Anna V. Bilous
Author:
Deepto Chakrabarty
Author:
Keith C. Gendreau
Author:
Tolga Güver
Author:
Gaurava K. Jaisawal
Author:
Erik Kuulkers
Author:
Christian Malacaria
Author:
Mason Ng
Author:
Andrea Sanna
Author:
Tod E. Strohmayer
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