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Quest for the donor star in the magnetic precataclysmic variable V1082 Sgr

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Date
10/12/2018
Author
Tovmassian, G.
González, J. F.
Hernández, M.-S.
González–Buitrago, D.
Zharikov, S.
Hernández Santisteban, J. V.
Keywords
Binaries: close
Novae
Cataclysmic variables
Stars: individual: V1082 Sgr
Star: rotation
Stars: winds
Outflows
QB Astronomy
QC Physics
DAS
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Abstract
We obtained high-resolution spectra and multicolor photometry of V1082 Sgr to study the donor star in this 20.8 hr orbital period binary, which is assumed to be a detached system. We measured the rotational velocity (v sin i = 26.5 ± 2.0 km s−1), which, coupled with the constraints on the white dwarf mass from the X-ray spectroscopy, leads to the conclusion that the donor star barely fills 70% of its corresponding Roche lobe radius. It appears to be a slightly evolved K2-type star. This conclusion was further supported by a recently published distance to the binary system measured by the Gaia mission. At the same time, it becomes difficult to explain a very high (>10−9 M⊙ yr-1 ) mass transfer and mass accretion rate in a detached binary via stellar wind and magnetic coupling.
Citation
Tovmassian , G , González , J F , Hernández , M-S , González–Buitrago , D , Zharikov , S & Hernández Santisteban , J V 2018 , ' Quest for the donor star in the magnetic precataclysmic variable V1082 Sgr ' , Astrophysical Journal , vol. 869 , no. 1 , 22 . https://doi.org/10.3847/1538-4357/aaec02
Publication
Astrophysical Journal
Status
Peer reviewed
DOI
https://doi.org/10.3847/1538-4357/aaec02
ISSN
0004-637X
Type
Journal article
Rights
Copyright © 2018 American Astronomical Society. All rights reserved. This work has been made available online in accordance with publisher policies or with permission. Permission for further reuse of this content should be sought from the publisher or the rights holder. This is the final published version of the work, which was originally published at https://doi.org/10.3847/1538-4357/aaec02
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  • University of St Andrews Research
URL
https://arxiv.org/abs/1811.08049
http://adsabs.harvard.edu/abs/2018ApJ...869...22T
URI
http://hdl.handle.net/10023/18455

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