SEARCH FOR P-MODE PULSATIONS IN LATE-TYPE CP STARS

The Sun, solar-like oscillators, δ-Scuti and roAp stars are few examples of the main-sequence pulsating stars for which the quantitative measurements of the internal structure parameters have been derived from their oscillations. For the asteroseismic study of δ-Sct and roAp stars, a project the “Nainital-Cape Survey” is being run at ARIES, Nainital since 1999. In this paper, we present the overview of stellar-seismology and briefly describe the results obtained under the survey project.