Properties of He-rich stars. IV. Search for He vertical stratification

Details Properties of He-rich stars. IV. Search for He vertical stratification Properties of He-rich stars. IV. Search for He vertical stratification

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ap%26ss.332..163z&link_type=abstract

Astrophysics and Space Science, Volume 332, Issue 1, pp.163-170

Astronomy and Astrophysics

Astrophysics

Stars, Early Type, Atmosphere, Abundances

Scientific paper

The study of He-r stellar photospheres aiming at detection of vertical stratification of helium is presented. Using high resolution data and the spectrum synthesis method, helium enhancement was indicated in several stars in a sample and in the two He layer model (minimum model), and it is suggested for the photosphere. The break point of helium abundance is often around a depth-mass variable of 0.2. The He-r stars are slightly evolved, the interval of the surface gravities being (3.8-4.2), in agreement with standard B type stars. The giant star HD68450 possesses a strong vertical stratification of helium. Previous reports on the elemental stratification were confirmed for our sample.

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