Spectroscopic observations of SPB and challenges to asteroseismology in solar-type stars

Details Spectroscopic observations of SPB and challenges to asteroseismology in solar-type stars Spectroscopic observations of SPB and challenges to asteroseismology in solar-type stars

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003asthe..96..321m&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 96, No. 6, p. 321 - 327 (2003)

Mathematics

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Solar-Type Stars, Asteroseismology, Pulsating Stars

Scientific paper

The HIDES has enabled us to make systematic observations of variable stars with smaller amplitudes, including nonradially pulsating variable stars in particular. In this article, we briefly summarize such pulsating stars, and then introduce our observations with HIDES on the new class of pulsating stars, SPB (Slowly Pulsating B stars). We also mention our challenges to detect tiny oscillations in solar-type stars with the iodine cell toward their asteroseismological study.

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