Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...105..133b&link_type=abstract
Astronomy and Astrophysics, vol. 105, no. 1, Jan. 1982, p. 133-139.
Astronomy and Astrophysics
Astrophysics
14
Dynamo Theory, Giant Stars, Late Stars, Stellar Magnetic Fields, Stellar Rotation, X Rays, Convection, Emission Spectra, Solar Flux, Stellar Luminosity, Stellar Models, Thermal Energy
Scientific paper
The observations of X-ray emission from late type main sequence and giant stars show that a coronal heating due to acoustic waves is unlikely.
As suggested by Vaiana and Rosner, the conversion of magnetic into thermal energy may be responsible for the X-ray emission from such a kind of stars.
The proposed ingredients in our analysis are the differential rotation and dynamo action which are able to generate a magnetic activity at the star's surface which in turn gives rise to the observed X-ray emission. We assume that the interaction of rotation with convection, in stars possessing outer convective envelopes, is the dominant mechanism for generating differential rotation and dynamo action, and that the stressing of the coronal magnetic flux tubes by the surface turbulence, converting magnetic into thermal energy, determine the level of X-ray emission.
Therefore we compute a series of models of luminosity class III giant stars, and determine the surface X-ray flux.
Comparing these results with those concerning the late type main sequence star models, previously computed by the same authors, and with observations, it appears that the proposed mechanism is plausible.
Belvedere Gaetano
Chiuderi Claudio
Paterno' Lucio
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