Structure of the atmosphere of the magnetic star hd21699

Details Structure of the atmosphere of the magnetic star hd21699 Structure of the atmosphere of the magnetic star hd21699

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012ap.....55..140g&link_type=abstract

Astrophysics, Volume 55, Issue 1, pp.140-143

Astronomy and Astrophysics

Astrophysics

Scientific paper

The temperature distribution with depth in the atmosphere of the magnetic star HD21699 is modelled for each observed rotational phase using Hδ line profiles obtained with a signal to noise ratio S/N = 1000. The observed temperature distributions were averaged within and outside the region of the magnetic spots. It appears that these average temperatures are equal to within the limits of error. This shows that the magnetic field does not affect the physical condition of the matter in the star and does not disturb its thermodynamic state.

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