SKARKA, Marek, Petr KABÁTH, Ernst PAUNZEN, Martin MAŠEK, Jiří ŽÁK and Jan JANÍK. On the first delta Scuti-like pulsating Ap star in an eclipsing binary. Contributions of the Astronomical Observatory Skalnaté Pleso. Tatranská Lomnica: Astronomical Institute, Slovak Academy of Sciences, 2020, vol. 50, No 2, p. 630-631. ISSN 1335-1842. Available from: https://dx.doi.org/10.31577/caosp.2020.50.2.630.
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Basic information
Original name On the first delta Scuti-like pulsating Ap star in an eclipsing binary
Authors SKARKA, Marek (203 Czech Republic, guarantor, belonging to the institution), Petr KABÁTH (203 Czech Republic), Ernst PAUNZEN (40 Austria, belonging to the institution), Martin MAŠEK (203 Czech Republic), Jiří ŽÁK (203 Czech Republic, belonging to the institution) and Jan JANÍK (203 Czech Republic, belonging to the institution).
Edition Contributions of the Astronomical Observatory Skalnaté Pleso, Tatranská Lomnica, Astronomical Institute, Slovak Academy of Sciences, 2020, 1335-1842.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher Slovakia
Confidentiality degree is not subject to a state or trade secret
WWW URL
Impact factor Impact factor: 0.316
RIV identification code RIV/00216224:14310/20:00115533
Organization unit Faculty of Science
Doi http://dx.doi.org/10.31577/caosp.2020.50.2.630
UT WoS 000523574300055
Keywords (in Czech) Stars: HD99458; Stars: chemically peculiar; binaries: eclipsing; Stars: pulsations
Keywords in English Stars: HD99458; Stars: chemically peculiar; binaries: eclipsing; Stars: pulsations
Tags rivok
Tags International impact, Reviewed
Changed by Changed by: Mgr. Marie Šípková, DiS., učo 437722. Changed: 24/11/2020 13:35.
Abstract
HD99458 was recently discovered to be a first object of its kind: a short-period eclipsing binary hosts a spotted, chemically peculiar A-type primary star that is a delta Scuti pulsator, and an M-dwarf secondary. These phenomena should not co-exist at the same time. Based on new photometric data we find that the previously published period of the main pulsation mode is a Nyquist alias of the true period (0.036 d, and not 0.052 d) given by the Kepler sampling.
Links
EF16_027/0008360, research and development projectName: Postdoc@MUNI
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