TV Cassiopeiae with Chandra and XMM–Newton X-ray Observations

TV Cassiopeia (TV Cas) is a well-known eclipsing Algol-type binary comprising a B9V primary and F7 IV secondary in an orbit with a period of 1.81 days, together with a purported low-mass companion in a wide orbit. Despite the considerable attention TV Cas has received in optical and UV bands, no X-r...

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Main Authors: Yang, Jun, Drake, Jeremy J., Wik, Daniel R., Laycock, Silas G. T.
Other Authors: MIT Kavli Institute for Astrophysics and Space Research
Format: Article
Published: MDPI AG 2020
Online Access:https://hdl.handle.net/1721.1/124964
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author Yang, Jun
Drake, Jeremy J.
Wik, Daniel R.
Laycock, Silas G. T.
author2 MIT Kavli Institute for Astrophysics and Space Research
author_facet MIT Kavli Institute for Astrophysics and Space Research
Yang, Jun
Drake, Jeremy J.
Wik, Daniel R.
Laycock, Silas G. T.
author_sort Yang, Jun
collection MIT
description TV Cassiopeia (TV Cas) is a well-known eclipsing Algol-type binary comprising a B9V primary and F7 IV secondary in an orbit with a period of 1.81 days, together with a purported low-mass companion in a wide orbit. Despite the considerable attention TV Cas has received in optical and UV bands, no X-ray analysis has been reported. Chandra has detected TV Cas six times and XMM–Newton observed it twice, all serendipitously during observations of the starburst galaxy IC 10. We have put all the X-ray data together to investigate its coronal morphology and spectral properties. We use the X-ray light curves and eclipses to probe the emitting geometry and the X-ray spectra at different epochs to investigate the activity mechanisms and test speculation that TV Cas undergoes significant mass transfer episodes.
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spelling mit-1721.1/1249642022-09-26T17:29:47Z TV Cassiopeiae with Chandra and XMM–Newton X-ray Observations Yang, Jun Drake, Jeremy J. Wik, Daniel R. Laycock, Silas G. T. MIT Kavli Institute for Astrophysics and Space Research TV Cassiopeia (TV Cas) is a well-known eclipsing Algol-type binary comprising a B9V primary and F7 IV secondary in an orbit with a period of 1.81 days, together with a purported low-mass companion in a wide orbit. Despite the considerable attention TV Cas has received in optical and UV bands, no X-ray analysis has been reported. Chandra has detected TV Cas six times and XMM–Newton observed it twice, all serendipitously during observations of the starburst galaxy IC 10. We have put all the X-ray data together to investigate its coronal morphology and spectral properties. We use the X-ray light curves and eclipses to probe the emitting geometry and the X-ray spectra at different epochs to investigate the activity mechanisms and test speculation that TV Cas undergoes significant mass transfer episodes. 2020-04-30T21:24:28Z 2020-04-30T21:24:28Z 2019-10 Article http://purl.org/eprint/type/ConferencePaper 2504-3900 https://hdl.handle.net/1721.1/124964 Yang, Jun et al. "TV Cassiopeiae with Chandra and XMM–Newton X-ray Observations" Proceedings of Recent Progress in Relativistic Astrophysics 17, 1 (October 2019) © 2019 The Authors http://dx.doi.org/10.3390/proceedings2019017010 Proceedings of Recent Progress in Relativistic Astrophysics Creative Commons Attribution 4.0 International license https://creativecommons.org/licenses/by/4.0/ application/pdf MDPI AG MDPI
spellingShingle Yang, Jun
Drake, Jeremy J.
Wik, Daniel R.
Laycock, Silas G. T.
TV Cassiopeiae with Chandra and XMM–Newton X-ray Observations
title TV Cassiopeiae with Chandra and XMM–Newton X-ray Observations
title_full TV Cassiopeiae with Chandra and XMM–Newton X-ray Observations
title_fullStr TV Cassiopeiae with Chandra and XMM–Newton X-ray Observations
title_full_unstemmed TV Cassiopeiae with Chandra and XMM–Newton X-ray Observations
title_short TV Cassiopeiae with Chandra and XMM–Newton X-ray Observations
title_sort tv cassiopeiae with chandra and xmm newton x ray observations
url https://hdl.handle.net/1721.1/124964
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