Spectroscopic Survey of δ SCT Stars

Details Spectroscopic Survey of δ SCT Stars Spectroscopic Survey of δ SCT Stars

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap%26ss.263..267s&link_type=abstract

Astrophysics and Space Science, v. 263, Issue 1/4, p. 267-270 (1998).

Astronomy and Astrophysics

Astrophysics

Scientific paper

The methods used to derive effective temperatures, projected rotational velocities and surface gravities of a sample of low and high-amplitude δ Sct stars are presented here. Effective temperatures were derived using Hα and Hβ line profiles whereas rotational velocities were calculated following the method described in Solano & Fernley (1997). Surface gravities were obtained using Hipparcos parallaxes and evolutionary models (Claret 1995). The results of this analysis will be published in a subsequent paper (Solano & Pintado 1999).

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