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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: A PATT Linked Grant for Sheffield Astrophysics 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