Mode identification in the pulsating subdwarf Balloon 090100001 by means of the spectrophotometric method

Details Mode identification in the pulsating subdwarf Balloon 090100001 by means of the spectrophotometric method Mode identification in the pulsating subdwarf Balloon 090100001 by means of the spectrophotometric method

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007coast.150..263b&link_type=abstract

Communications in Astroseismology, Vol. 150, p.263

Astronomy and Astrophysics

Astronomy

Scientific paper

We present the first successful application of the spectrophotometric
method of mode identification to a pulsating subdwarf B star, Balloon
090100001. We confirm that the dominant mode is radial and that the
observed triplet can be interpreted in terms of a rotationally split
dipole mode.

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