The sdB pulsating star V391 Peg and its putative giant planet revisited after 13 years of time-series photometric data (2018)

First Author: Silvotti R
Attributed to:  Warwick Astronomy and Astrophysics Consolidated Grant 2017-2020 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/201731473

Publication URI: http://dx.doi.org/10.1051/0004-6361/201731473

Type: Journal Article/Review

Parent Publication: Astronomy & Astrophysics