The sdB pulsating star V391 Peg and its putative giant planet revisited after 13 years of time-series photometric data

Silvotti, R., Schuh, S., Kim, S.-L. et al. (10 more authors) (2018) The sdB pulsating star V391 Peg and its putative giant planet revisited after 13 years of time-series photometric data. Astronomy and Astrophysics , 611. A85. ISSN 0004-6361

Abstract

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Authors/Creators:
Copyright, Publisher and Additional Information: Reproduced with permission from Astronomy & Astrophysics, © ESO 2018.
Keywords: stars: horizontal-branch; stars: oscillations; asteroseismology; stars: individual: V391 Peg; planets and satellites: detection; planets and satellites: individual: V391 Peg b
Dates:
  • Published: 4 April 2018
  • Accepted: 3 November 2017
Institution: The University of Sheffield
Academic Units: The University of Sheffield > Faculty of Science (Sheffield) > Department of Physics and Astronomy (Sheffield)
Funding Information:
FunderGrant number
SCIENCE AND TECHNOLOGY FACILITIES COUNCILST/M001350/1
Depositing User: Symplectic Sheffield
Date Deposited: 30 Apr 2018 13:53
Last Modified: 30 Apr 2018 13:53
Published Version: https://doi.org/10.1051/0004-6361/201731473
Status: Published
Publisher: EDP Sciences
Refereed: Yes
Identification Number: https://doi.org/10.1051/0004-6361/201731473
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