Multi-site Photometry of the Pulsating White Dwarf G38-29

Details Multi-site Photometry of the Pulsating White Dwarf G38-29 Multi-site Photometry of the Pulsating White Dwarf G38-29

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...211.1510t&link_type=abstract

American Astronomical Society, AAS Meeting #211, #15.10; Bulletin of the American Astronomical Society, Vol. 39, p.765

Astronomy and Astrophysics

Astronomy

Scientific paper

In November 2007 the Delaware Asteroseismic Research Center (DARC) initiated a multi-site campaign on the large amplitude pulsating white dwarf star G38-29. The purpose of these observations is to measure the star's complex set of pulsation periods. With precise period measurements and a high S/N light curve, we can measure the properties of this star's outer convection zone by utilizing the technique of Montgomery (2005). Here we present the preliminary light curve, Fourier transform, and period analysis from these observations of G38-29.
This work was primarily funded by the Delaware Asteroseismic Research Center located at Mount Cuba Observatory.

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