The Nainital-Cape Survey-III : A Search for Pulsational Variability in Chemically Peculiar Stars

TL;DR

The Nainital-Cape Survey-III investigates pulsational variability in chemically peculiar stars using high-speed photometry, confirming known pulsations and providing a catalog of null results to understand stellar pulsation characteristics.

Contribution

This study presents new high-precision photometric data confirming pulsations in specific chemically peculiar stars and offers a comprehensive catalog of null results for the first time.

Findings

Confirmed pulsational period of HD25515 as 2.78 hours.

Detected known frequencies in HD113878 and HD118660.

Compiled a catalog of 61 null-result stars with 87 frequency spectra.

Abstract

The Nainital-Cape survey is a dedicated research programme to search and study pulsational variability in chemically peculiar stars in the Northern Hemisphere. The aim of the survey is to search such chemically peculiar stars which are pulsationally unstable. The observations of the sample stars were carried out in high-speed photometric mode using a three-channel fast photometer attached to the 1.04-m Sampurnanand telescope at ARIES. The new photometric observations confirmed that the pulsational period of star HD25515 is 2.78-hrs. The repeated time-series observations of HD113878 and HD118660 revealed that previously known frequencies are indeed present in the new data sets. We have estimated the distances, absolute magnitudes, effective temperatures and luminosities of these stars. Their positions in the H-R diagram indicate that HD25515 and HD118660 lie near the main-sequence while HD113878 is an evolved star. We also present a catalogue of 61 stars classified as null results, along with the corresponding 87 frequency spectra taken over the time scale 2002-2008. A statistical analysis of these null results shows, by comparison with past data, that the power of the noise in the light curves has slightly increased during the last few years.