The complex coronal structure of the Oe star HD 175754

Details The complex coronal structure of the Oe star HD 175754 The complex coronal structure of the Oe star HD 175754

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003pobeo..76..175d&link_type=abstract

Publications of the Astronomical Observatory of Belgrade (ISSN 0373-3742), No. 76, p. 175 - 178 (2003). In: IV Serbian Conferenc

Astronomy and Astrophysics

Astronomy

O Supergiants, Coronal Structure

Scientific paper

We present the study of the HD 175754 coronal regions, based on the model proposed by Danezis et al. (2003). By this model, we can calculate, for all the independent density regions, the apparent expansion/contraction velocities (Vexp), the apparent rotation velocities (Vrot), as well as the values of ξ, which is an expression of the optical depth.

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