Rebassa-Mansergas, A., Parsons, S.G., Dhillon, V.S. orcid.org/0000-0003-4236-9642 et al. (4 more authors)
(2019)
Accurate mass and radius determinations of a cool subdwarf in an eclipsing binary.
Nature Astronomy, 3 (6).
pp. 553-560.
ISSN 2397-3366
Abstract
Cool subdwarfs are metal-poor low-mass stars that formed during the early stages of the evolution of our Galaxy. Because they are relatively rare in the vicinity of the Sun, we know of few cool subdwarfs in the solar neighbourhood, and none for which both the mass and the radius are accurately determined. This hampers our understanding of stars at the low-mass end of the main sequence. Here we report the discovery of SDSSJ235524.29+044855.7 as an eclipsing binary containing a cool subdwarf star, with a white dwarf companion. From the light curve and the radial-velocity curve of the binary we determine the mass and the radius of the cool subdwarf and we derive its effective temperature and luminosity by analysing its spectral energy distribution. Our results validate the theoretical relations between mass, radius, effective temperature and luminosity for low-mass, low-metallicity stars.
Metadata
Item Type: | Article |
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Authors/Creators: |
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Copyright, Publisher and Additional Information: | © The Author(s), under exclusive licence to Springer Nature Limited 2019. This is an author-produced version of a paper subsequently published in Nature Astronomy. Uploaded in accordance with the publisher's self-archiving policy. |
Dates: |
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Institution: | The University of Sheffield |
Academic Units: | The University of Sheffield > Faculty of Science (Sheffield) > Department of Physics and Astronomy (Sheffield) |
Funding Information: | Funder Grant number EUROPEAN RESEARCH COUNCIL HiPERCAM - 340040 |
Depositing User: | Symplectic Sheffield |
Date Deposited: | 18 Mar 2019 16:37 |
Last Modified: | 19 Nov 2021 13:49 |
Status: | Published |
Publisher: | Nature Research |
Refereed: | Yes |
Identification Number: | 10.1038/s41550-019-0746-7 |
Related URLs: | |
Open Archives Initiative ID (OAI ID): | oai:eprints.whiterose.ac.uk:143774 |