HD 99458: First time ever Ap-type star as a δ Scuti pulsator in a short period eclipsing binary?. Issue 3 (3rd June 2019)

• Record Type: Journal Article
• Authors: Skarka, M; Kabáth, P; Paunzen, E; Fedurco, M; Budaj, J; Dupkala, D; Krtička, J; Hatzes, A; Pribulla, T; Parimucha, Š; Mikulášek, Z; Guenther, E; Sabotta, S; Blažek, M; Dvořáková, J; Hambálek, L; Klocová, T; Kollár, V; Kundra, E; Šlechta, M; Vaňko, M
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 487:Issue 3(2019)
• Page Start: 4230
• Page End: 4237
• Publication Date: 2019-06-03
• Subjects: techniques: photometric -- techniques: spectroscopic -- binaries: eclipsing -- stars: chemically peculiar -- stars: individual: HD 99458 -- stars: oscillations; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stz1478
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: We present the discovery of a unique object, a chemically peculiar Ap-type star showing δ 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 δ Scuti type are also extremely rare among CP2 stars and no unambiguously proven candidate has been reported. HD 99458 was formerly thought to be 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 2 = 0.45(2) M⊙ ) 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.