Photometric and spectroscopic variability of 53 Per

Date Issued
2017
Author(s)
Niemczura, E.
•
Pigulski, A.
•
Lehmann, H.
•
Kamiński, K.
•
•
Stateva, I.
•
Napetova, M.
Abstract
A new investigation of the variability of the SPB-type star 53 Per is presented. The analysis of the BRITE photometry allowed us to determine eight independent frequencies and the combination one. Five of these frequencies and the combination frequency were not known before. In addition, we gathered more than 1800 new moderate and high-resolution spectra of 53 Per spread over approximately six months. Their frequency analysis revealed four independent frequencies and the combination frequency, all consistent with the BRITE results.
Coverage
Second BRITE-Constellation Science Conference: Small Satellites - Big Science
All editors
Zwintz, Konstanze; Poretti, Ennio
Series
Volume
5
Start page
217
Conferenece
Second BRITE-Constellation Science Conference: Small satellites—big science
Conferenece place
Innsbruck
Conferenece date
22–26 August, 2016
Uri
Url
Issn Identifier
2545-1022
Ads BibCode
2017sbcs.conf..217N
Rights
open.access
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