Benkő, József and Sódor, Ádám and Pál, András (2021) Photometric and Spectroscopic Investigations of the Galactic Field RRc Candidates V764 Mon and HY Com. ACTA ASTRONOMICA, 71. pp. 55-71. ISSN 0001-5237
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Abstract
By analyzing photometric and spectroscopic time series, we show that the pulsator V764 Mon, assumed to be the brightest RR Lyr star in the sky, is in fact a rapidly rotating δ Sct star with an unusually long dominant period (P1=0.29 d). Our spectroscopy confirmed the binarity of V764 Mon discovered by the Gaia satellite. In the case of HY Com, a bona fide RRc star, we present its first complete radial velocity curve. Additionally, we found that the star continues its strong phase variation reported before.
Item Type: | Article |
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Uncontrolled Keywords: | Astrophysics - Solar and Stellar Astrophysics; Stars: oscillations - Stars: variables: RR Lyrae - Stars: variables: delta Scuti - Methods: data analysis - Space vehicles; |
Subjects: | Q Science / természettudomány > QB Astronomy, Astrophysics / csillagászat, asztrofizika |
SWORD Depositor: | MTMT SWORD |
Depositing User: | MTMT SWORD |
Date Deposited: | 17 Jan 2023 14:23 |
Last Modified: | 17 Jan 2023 14:23 |
URI: | http://real.mtak.hu/id/eprint/156701 |
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