SKARKA, Marek, Petr KABÁTH, Ernst PAUNZEN, Miroslav FEDURCO, Ján BUDAJ, Daniel DUPKALA, Jiří KRTIČKA, Artie P. HATZES, Theodor PRIBULLA, Š. PARIMUCHA, Zdeněk MIKULÁŠEK, E. GUENTHER, Silvia SABOTTA, Martin BLAŽEK, Jana DVOŘÁKOVÁ, L. HAMBÁLEK, Tereza KLOCOVÁ, V. KOLLÁR, E. KUNDRA, M. ŠLECHTA and M. VAŇKO. HD 99458: First time ever Ap-type star as a S Scuti pulsator in a short period eclipsing binary? Monthly Notices of the Royal Astronomical Society. Oxford: OXFORD UNIV PRESS, 2019, vol. 487, No 3, p. 4230-4237. ISSN 0035-8711. Available from: https://dx.doi.org/10.1093/mnras/stz1478.
Other formats:   BibTeX LaTeX RIS
Basic information
Original name HD 99458: First time ever Ap-type star as a S Scuti pulsator in a short period 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), Miroslav FEDURCO (703 Slovakia), Ján BUDAJ (703 Slovakia), Daniel DUPKALA, Jiří KRTIČKA (203 Czech Republic, belonging to the institution), Artie P. HATZES, Theodor PRIBULLA, Š. PARIMUCHA, Zdeněk MIKULÁŠEK (203 Czech Republic, belonging to the institution), E. GUENTHER, Silvia SABOTTA, Martin BLAŽEK (203 Czech Republic, belonging to the institution), Jana DVOŘÁKOVÁ, L. HAMBÁLEK, Tereza KLOCOVÁ, V. KOLLÁR, E. KUNDRA, M. ŠLECHTA and M. VAŇKO.
Edition Monthly Notices of the Royal Astronomical Society, Oxford, OXFORD UNIV PRESS, 2019, 0035-8711.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher United Kingdom of Great Britain and Northern Ireland
Confidentiality degree is not subject to a state or trade secret
WWW Full Text
Impact factor Impact factor: 5.357
RIV identification code RIV/00216224:14310/19:00107454
Organization unit Faculty of Science
Doi http://dx.doi.org/10.1093/mnras/stz1478
UT WoS 000478053200094
Keywords in English techniques; photometric techniques; spectroscopic binaries; eclipsing stars; chemically peculiar stars; individual; 99458 stars; oscillations
Tags rivok
Tags International impact, Reviewed
Changed by Changed by: Mgr. Marie Šípková, DiS., učo 437722. Changed: 10/3/2020 10:15.
Abstract
We present the discovery of a unique object, a chemically peculiar Ap-type star showing fi Scuti pulsations that, is bound in an eclipsing binary system with an orbital period shorter than 3 d. HD 99458 is therefore a complex astrophysical laboratory opening doors for studying various, often contradictory, physical phenomena at the same time. It is the first Ap star ever discovered in an eclipsing binary. The orbital period of 2.722 d is the second shortest among all known chemically peculiar (CP2) binary stars. Pulsations of (S Scuti type are also extremely rare among CP2 stars and no unambiguously proven candidate has been reported. HD 99458 was formerly thought to he a star hosting an exoplanet, but we definitely reject this hypothesis using photometric observations from the K2 mission and new radial velocity measurements. The companion is a low-mass red dwarf star (M? = 0.45(2)Mo) on an inclined orbit (i = 73.2(6) deg) that shows only grazing eclipses. The rotation and orbital periods are synchronized, while the rotation and orbital axes are misaligned. HD 99458 is an interesting system deserving of more intense investigations.
Links
EF16_027/0008360, research and development projectName: Postdoc@MUNI
GA18-05665S, research and development projectName: Ztráta hmoty v pozdních fázích vývoje hmotných hvězd
Investor: Czech Science Foundation
PrintDisplayed: 4/5/2024 14:59