The University of Southampton
University of Southampton Institutional Repository

A NICER discovery of a low-frequency quasi-periodic oscillation in the soft-intermediate state of MAXI J1535-571

A NICER discovery of a low-frequency quasi-periodic oscillation in the soft-intermediate state of MAXI J1535-571
A NICER discovery of a low-frequency quasi-periodic oscillation in the soft-intermediate state of MAXI J1535-571

We present the discovery of a low-frequency ≈5.7 Hz quasi-periodic oscillation (QPO) feature in observations of the black hole X-ray binary MAXI J1535-571 in its soft-intermediate state, obtained in 2017 September-October by the Neutron Star Interior Composition Explorer. The feature is relatively broad (compared to other low-frequency QPOs; quality factor Q ≈ 2) and weak (1.9% rms in 3-10 keV), and is accompanied by a weak harmonic and low-amplitude broadband noise. These characteristics identify it as a weak Type A/B QPO, similar to ones previously identified in the soft-intermediate state of the transient black hole X-ray binary XTE J1550-564. The lag-energy spectrum of the QPO shows increasing soft lags toward lower energies, approaching 50 ms at 1 keV (with respect to a 3-10 keV continuum). This large phase shift has similar amplitude but opposite sign to that seen in Rossi X-Ray Timing Explorer data for a Type B QPO from the transient black hole X-ray binary GX 339-4. Previous phase-resolved spectroscopy analysis of the Type B QPO in GX 339-4 pointed toward a precessing jet-like corona illuminating the accretion disk as the origin of the QPO signal. We suggest that this QPO in MAXI J1535-571 may have the same origin, with the different lag sign depending on the scale height of the emitting region and the observer inclination angle.

accretion, accretion disks, black hole physics, stars: black holes, X-rays: binaries, X-rays: individual (MAXI J1535)
2041-8205
Stevens, A. L.
8ec4653d-0ea7-46a8-9d3f-807e57a2da93
Uttley, P.
db770bd7-d97e-43f5-99d4-a585bccd352a
Altamirano, D.
d5ccdb09-0b71-4303-9538-05b467be075b
Arzoumanian, Z.
5befbba6-f6a1-47c8-ae9e-021c5d854a64
Bult, P.
73bd0a3d-c566-4046-86c9-31f6e6cdac07
Cackett, E. M.
db500756-c971-444b-9677-4ee742b2dac5
Fabian, A. C.
b9bef0bc-2ecd-49dc-ab2b-954cabea88ba
Gendreau, K. C.
cad26609-b22d-4c1d-ada3-4af51e2cd780
Ha, K. Q.
bc892b91-0064-490f-8e4f-6507070f3a00
Homan, J.
549baf32-2442-4247-824e-21bb018b05f5
Ingram, A. R.
af60eb4b-a6ff-4d75-a0f8-07cd27f28611
Kara, E.
dcf44b44-cf7f-4bbe-9254-9c55741365b0
Kellogg, J.
ea44fbe7-8071-4683-a90f-324c961e8b73
Ludlam, R. M.
b27b6ff8-9743-49f2-833a-115803efa43a
Miller, J. M.
be4c8f0f-91e6-47de-9d38-235a632d8b90
Neilsen, J.
08c1d837-abeb-4a7d-bf2a-3a0fc6479110
Pasham, D. R.
0205c46d-c904-447e-9846-1b198d64ff7d
Remillard, R. A.
87600a84-66cb-400a-97d2-f61e7a7206c3
Steiner, J. F.
9001e118-7c30-4295-af66-7ce9c3a3701b
Eijnden, J. Van Den
abb08069-7f5c-430a-a68f-6ff0bb0d920a
Stevens, A. L.
8ec4653d-0ea7-46a8-9d3f-807e57a2da93
Uttley, P.
db770bd7-d97e-43f5-99d4-a585bccd352a
Altamirano, D.
d5ccdb09-0b71-4303-9538-05b467be075b
Arzoumanian, Z.
5befbba6-f6a1-47c8-ae9e-021c5d854a64
Bult, P.
73bd0a3d-c566-4046-86c9-31f6e6cdac07
Cackett, E. M.
db500756-c971-444b-9677-4ee742b2dac5
Fabian, A. C.
b9bef0bc-2ecd-49dc-ab2b-954cabea88ba
Gendreau, K. C.
cad26609-b22d-4c1d-ada3-4af51e2cd780
Ha, K. Q.
bc892b91-0064-490f-8e4f-6507070f3a00
Homan, J.
549baf32-2442-4247-824e-21bb018b05f5
Ingram, A. R.
af60eb4b-a6ff-4d75-a0f8-07cd27f28611
Kara, E.
dcf44b44-cf7f-4bbe-9254-9c55741365b0
Kellogg, J.
ea44fbe7-8071-4683-a90f-324c961e8b73
Ludlam, R. M.
b27b6ff8-9743-49f2-833a-115803efa43a
Miller, J. M.
be4c8f0f-91e6-47de-9d38-235a632d8b90
Neilsen, J.
08c1d837-abeb-4a7d-bf2a-3a0fc6479110
Pasham, D. R.
0205c46d-c904-447e-9846-1b198d64ff7d
Remillard, R. A.
87600a84-66cb-400a-97d2-f61e7a7206c3
Steiner, J. F.
9001e118-7c30-4295-af66-7ce9c3a3701b
Eijnden, J. Van Den
abb08069-7f5c-430a-a68f-6ff0bb0d920a

Stevens, A. L., Uttley, P., Altamirano, D., Arzoumanian, Z., Bult, P., Cackett, E. M., Fabian, A. C., Gendreau, K. C., Ha, K. Q., Homan, J., Ingram, A. R., Kara, E., Kellogg, J., Ludlam, R. M., Miller, J. M., Neilsen, J., Pasham, D. R., Remillard, R. A., Steiner, J. F. and Eijnden, J. Van Den (2018) A NICER discovery of a low-frequency quasi-periodic oscillation in the soft-intermediate state of MAXI J1535-571. Astrophysical Journal Letters, 865 (2), [L15]. (doi:10.3847/2041-8213/aae1a4).

Record type: Article

Abstract

We present the discovery of a low-frequency ≈5.7 Hz quasi-periodic oscillation (QPO) feature in observations of the black hole X-ray binary MAXI J1535-571 in its soft-intermediate state, obtained in 2017 September-October by the Neutron Star Interior Composition Explorer. The feature is relatively broad (compared to other low-frequency QPOs; quality factor Q ≈ 2) and weak (1.9% rms in 3-10 keV), and is accompanied by a weak harmonic and low-amplitude broadband noise. These characteristics identify it as a weak Type A/B QPO, similar to ones previously identified in the soft-intermediate state of the transient black hole X-ray binary XTE J1550-564. The lag-energy spectrum of the QPO shows increasing soft lags toward lower energies, approaching 50 ms at 1 keV (with respect to a 3-10 keV continuum). This large phase shift has similar amplitude but opposite sign to that seen in Rossi X-Ray Timing Explorer data for a Type B QPO from the transient black hole X-ray binary GX 339-4. Previous phase-resolved spectroscopy analysis of the Type B QPO in GX 339-4 pointed toward a precessing jet-like corona illuminating the accretion disk as the origin of the QPO signal. We suggest that this QPO in MAXI J1535-571 may have the same origin, with the different lag sign depending on the scale height of the emitting region and the observer inclination angle.

Text
A NICER Discovery of a Low-frequency Quasi-periodic Oscillation in the Soft-intermediate State of MAXI J1535-571 - Accepted Manuscript
Download (976kB)

More information

Accepted/In Press date: 14 September 2018
e-pub ahead of print date: 26 September 2018
Published date: 1 October 2018
Keywords: accretion, accretion disks, black hole physics, stars: black holes, X-rays: binaries, X-rays: individual (MAXI J1535)

Identifiers

Local EPrints ID: 425558
URI: http://eprints.soton.ac.uk/id/eprint/425558
ISSN: 2041-8205
PURE UUID: 4b55d3eb-3178-4f67-a511-d331c60a1511
ORCID for D. Altamirano: ORCID iD orcid.org/0000-0002-3422-0074

Catalogue record

Date deposited: 24 Oct 2018 16:30
Last modified: 16 Nov 2024 05:01

Export record

Altmetrics

Contributors

Author: A. L. Stevens
Author: P. Uttley
Author: D. Altamirano ORCID iD
Author: Z. Arzoumanian
Author: P. Bult
Author: E. M. Cackett
Author: A. C. Fabian
Author: K. C. Gendreau
Author: K. Q. Ha
Author: J. Homan
Author: A. R. Ingram
Author: E. Kara
Author: J. Kellogg
Author: R. M. Ludlam
Author: J. M. Miller
Author: J. Neilsen
Author: D. R. Pasham
Author: R. A. Remillard
Author: J. F. Steiner
Author: J. Van Den Eijnden

Download statistics

Downloads from ePrints over the past year. Other digital versions may also be available to download e.g. from the publisher's website.

View more statistics

Atom RSS 1.0 RSS 2.0

Contact ePrints Soton: eprints@soton.ac.uk

ePrints Soton supports OAI 2.0 with a base URL of http://eprints.soton.ac.uk/cgi/oai2

This repository has been built using EPrints software, developed at the University of Southampton, but available to everyone to use.

We use cookies to ensure that we give you the best experience on our website. If you continue without changing your settings, we will assume that you are happy to receive cookies on the University of Southampton website.

×