TESS photometry of extreme helium stars PV Tel and V821 Cen

Author:

Jeffery C Simon1ORCID,Barentsen Geert2,Handler Gerald3

Affiliation:

1. Armagh Observatory and Planetarium, College Hill, Armagh BT61 9DG, UK

2. Bay Area Environmental Research Institute, PO Box 25, Moffett Field, CA 94035, USA

3. Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, ul. Bartycka 18, PL-00-716 Warsaw, Poland

Abstract

ABSTRACT PV Tel variables are extreme helium (EHe) stars known to be intrinsic light and velocity variable on characteristic time-scales of 0.1–25 d. With two exceptions, they are best described as irregular. Light curves have invariably been obtained from single-site terrestrial observatories. We present Transiting Exoplanet Survey Satellite observations of two bright EHe stars, Popper’s star (V821 Cen) and Thackeray’s star (PV Tel). PV Tel is variable on time-scales previously reported. V821 Cen is proven to be variable for the first time. Neither light curve shows any evidence of underlying regularity. Implications are considered.

Funder

NASA

Polish National Science Centre

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 4 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Period variability in the pulsating Extreme Helium stars V652 Her and BX Cir;Monthly Notices of the Royal Astronomical Society;2023-11-20

2. Asteroseismology Across the Hertzsprung–Russell Diagram;Annual Review of Astronomy and Astrophysics;2022-08-18

3. Detection of an extremely strong magnetic field in the double-degenerate binary merger product HD 144941;Monthly Notices of the Royal Astronomical Society;2021-07-28

4. TESS photometry of helium-rich hot subdwarfs: r modes in BD+37°442 and BD+37°1977;Monthly Notices of the Royal Astronomical Society;2020-06-04

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