An Investigation of Four Chemically Peculiar Stars with Photometric Periods below 12 Hours

TL;DR

This study investigates four chemically peculiar stars with short photometric periods, confirming their peculiar nature, analyzing their variability, and proposing pulsation or rotation as the underlying mechanisms, with one star being the shortest-period ACV variable known.

Contribution

The paper provides detailed analysis of four CP stars with periods below 12 hours, including new spectroscopic data and insights into their pulsational or rotational variability mechanisms.

Findings

HD 67983, HD 77013, and HD 81076 show pulsational variability.

HD 98000 exhibits the shortest known ACV period (~0.466 days).

The study links chemical peculiarities with pulsation and rotation in these stars.

Abstract

We present an investigation of three chemically peculiar (CP) stars and one CP star candidate which exhibit photometric periods below 12 hours. New spectroscopic observations have been acquired which confirm the peculiar nature of all objects. HD 77013 and HD 81076 are classical CP1 (Am) stars; HD 67983 is a marginal CP1 (Am: ) star, and HD 98000 is a CP2 (Ap) star. We have procured observations from the ASAS-3 and SuperWASP archives and obtained additional photometry in order to verify the results from the sky survey data. We have derived astrophysical parameters and investigated the positions of our target stars in the MBol versus log Teff diagram, from which information on evolutionary status has been derived. We present period analyses and discuss each object in detail. From the available data, we propose pulsational variability as the underlying mechanism for the variability in HD 67983, HD 77013 and HD 81076, which offer the opportunity to study the interaction of atomic diffusion and pulsation. HD 67983 and HD 77013 exhibit multiperiodic variability in the gamma Doradus frequency realm; HD 81076 is a delta Scuti star. The CP2 star HD 98000 exhibits monoperiodic variability with a frequency of f~2.148 c/d (P~0.466 d), which we interpret as the rotational period. If this assumption is correct, HD 98000 is the alpha2 Canum Venaticorum (ACV) variable with the shortest period hitherto observed and thus a very interesting object that might help to investigate the influence of rotational mixing on chemical peculiarities.