Monitoring observations of SMC X-1’s excursions (<scp>moose</scp>) III. X-ray spectroscopy of a warped, precessing accretion disc

ABSTRACT The moose (Monitoring Observations of SMC X-1’s Excursions) program uses the Neutron Star Interior Composition Explorer Mission (NICER) to monitor the high-mass X-ray binary SMC X-1 during its superorbital period excursions. Here, we perform X-ray spectral analyses of 26 NICER observations of SMC X-1, taken at the tail-end of the excursion between 2021-04-01 and 2022-01-05. We use a single spectral model to fit spectra observed in high, intermediate, and low states, using a combination of a partial covering fraction model, a blackbody disc, and a power-law component. We find that the partial covering fraction varies significantly with the superorbital state during superorbital excursion. Our findings suggest that the low/high state in SMC X-1 is caused by a very high obscuration of the accretion disc.

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Publication Details

Journal
Monthly Notices of the Royal Astronomical Society
Published
2024-12-04
DOI
https://doi.org/10.1093/mnras/stae2456
Citations
1
Primary Topic
Astrophysical Phenomena and Observations
Type
article
Field-Weighted Citation Impact
0.33

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article

Monitoring observations of SMC X-1’s excursions (moose) III. X-ray spectroscopy of a warped, precessing accretion disc

Rawan Karam, McKinley C. Brumback, B. E. Tetarenko, W. I. Clarkson et al.
1 citations
Monthly Notices of the Royal Astronomical Society
Astrophysical Phenomena and Observations
0.33
article

Monitoring observations of SMC X-1’s excursions (moose) III. X-ray spectroscopy of a warped, precessing accretion disc

Rawan Karam, McKinley C. Brumback, B. E. Tetarenko, W. I. Clarkson, Wasundara Athukoralalage, D. Altamirano, Arash Bahramian, Daryl Haggard, J. A. Kennea, Kristen C. Dage, Ryan C. Hickox, Chin‐Ping Hu, Joey Neilsen, P. A. Charles
article en
1 citations

Abstract

ABSTRACT The moose (Monitoring Observations of SMC X-1’s Excursions) program uses the Neutron Star Interior Composition Explorer Mission (NICER) to monitor the high-mass X-ray binary SMC X-1 during its superorbital period excursions. Here, we perform X-ray spectral analyses of 26 NICER observations of SMC X-1, taken at the tail-end of the excursion between 2021-04-01 and 2022-01-05. We use a single spectral model to fit spectra observed in high, intermediate, and low states, using a combination of a partial covering fraction model, a blackbody disc, and a power-law component. We find that the partial covering fraction varies significantly with the superorbital state during superorbital excursion. Our findings suggest that the low/high state in SMC X-1 is caused by a very high obscuration of the accretion disc.

Monthly Notices of the Royal Astronomical SocietyVol. 536(1)
Dartmouth College (US), Space Science Institute (US), Pennsylvania State University (US), Wayne State University (US), Middlebury College (US), University of Michigan (US), Center for Astrophysics Harvard & Smithsonian (US), University of Michigan–Dearborn (US), International Centre for Radio Astronomy Research (AU), University of Southampton (GB), McGill University (CA), National Changhua University of Education (TW), Université de Montréal (CA), Villanova University (US), Michigan State University (US)
National Aeronautics and Space Administration, McGill University, Space Telescope Science Institute, Canada Research Chairs, Nuclear Safety and Security Commission, National Science and Technology Council, Fonds de recherche du Québec, Goddard Space Flight Center, Natural Sciences and Engineering Research Council of Canada, Astrophysics Science Division
Openalex Percentile: Top 33%
Astrophysical Phenomena and Observations
0.33
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