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Simultaneous NICER and NuSTAR observations of the ultracompact x-ray binary 4U 0614+091

Simultaneous NICER and NuSTAR observations of the ultracompact x-ray binary 4U 0614+091
Simultaneous NICER and NuSTAR observations of the ultracompact x-ray binary 4U 0614+091
We present the first joint NuSTAR and NICER observations of the ultracompact X-ray binary 4U 0614+091. This source shows quasiperiodic flux variations on the timescale of ∼days. We use reflection modeling techniques to study various components of the accretion system as the flux varies. We find that the flux of the reflected emission and the thermal components representing the disk and the compact object trend closely with the overall flux. However, the flux of the power-law component representing the illuminating X-ray corona scales in the opposite direction, increasing as the total flux decreases. During the lowest flux observation, we see evidence of accretion disk truncation from roughly 6 gravitational radii to 11.5 gravitational radii. This is potentially analogous to the truncation seen in black hole low-mass X-ray binaries, which tends to occur during the low/hard state at sufficiently low Eddington ratios.
0004-637X
Moutard, D.L.
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Ludlam, R.M.
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García, J.A.
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Altamirano, D.
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Buisson, D.J.K.
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Cackett, E.M.
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Chenevez, J.
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Degenaar, N.
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Fabian, A.C.
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Homan, J.
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Jaodand, A.
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Pike, S.N.
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Shaw, A.W.
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Strohmayer, T.E.
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Tomsick, J.A.
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Coughenour, B.M.
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Moutard, D.L.
49936cb4-dd0f-48e6-8303-3708a528741c
Ludlam, R.M.
b27b6ff8-9743-49f2-833a-115803efa43a
García, J.A.
c9c5b240-fc95-4a3b-b79f-bc6e70ce876e
Altamirano, D.
d5ccdb09-0b71-4303-9538-05b467be075b
Buisson, D.J.K.
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Cackett, E.M.
db500756-c971-444b-9677-4ee742b2dac5
Chenevez, J.
25a95602-9e3d-4553-a442-5f4317ff2cd6
Degenaar, N.
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Fabian, A.C.
b9bef0bc-2ecd-49dc-ab2b-954cabea88ba
Homan, J.
549baf32-2442-4247-824e-21bb018b05f5
Jaodand, A.
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Pike, S.N.
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Shaw, A.W.
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Strohmayer, T.E.
491eee42-6b4e-4dcc-a7cd-2a36ac992a7d
Tomsick, J.A.
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Coughenour, B.M.
57954333-8ca2-4a94-a9c0-c0acc2a81861

Moutard, D.L., Ludlam, R.M., García, J.A., Altamirano, D., Buisson, D.J.K., Cackett, E.M., Chenevez, J., Degenaar, N., Fabian, A.C., Homan, J., Jaodand, A., Pike, S.N., Shaw, A.W., Strohmayer, T.E., Tomsick, J.A. and Coughenour, B.M. (2023) Simultaneous NICER and NuSTAR observations of the ultracompact x-ray binary 4U 0614+091. The Astrophysical Journal, 957 (27). (doi:10.3847/1538-4357/acf4f3).

Record type: Article

Abstract

We present the first joint NuSTAR and NICER observations of the ultracompact X-ray binary 4U 0614+091. This source shows quasiperiodic flux variations on the timescale of ∼days. We use reflection modeling techniques to study various components of the accretion system as the flux varies. We find that the flux of the reflected emission and the thermal components representing the disk and the compact object trend closely with the overall flux. However, the flux of the power-law component representing the illuminating X-ray corona scales in the opposite direction, increasing as the total flux decreases. During the lowest flux observation, we see evidence of accretion disk truncation from roughly 6 gravitational radii to 11.5 gravitational radii. This is potentially analogous to the truncation seen in black hole low-mass X-ray binaries, which tends to occur during the low/hard state at sufficiently low Eddington ratios.

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Accepted/In Press date: 28 August 2023
e-pub ahead of print date: 23 October 2023

Identifiers

Local EPrints ID: 490723
URI: http://eprints.soton.ac.uk/id/eprint/490723
ISSN: 0004-637X
PURE UUID: 0aa40d93-d4fb-44ed-9fbe-4c906fd64c95
ORCID for D. Altamirano: ORCID iD orcid.org/0000-0002-3422-0074

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Date deposited: 04 Jun 2024 16:57
Last modified: 16 Nov 2024 02:46

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Contributors

Author: D.L. Moutard
Author: R.M. Ludlam
Author: J.A. García
Author: D. Altamirano ORCID iD
Author: D.J.K. Buisson
Author: E.M. Cackett
Author: J. Chenevez
Author: N. Degenaar
Author: A.C. Fabian
Author: J. Homan
Author: A. Jaodand
Author: S.N. Pike
Author: A.W. Shaw
Author: T.E. Strohmayer
Author: J.A. Tomsick
Author: B.M. Coughenour

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