MAG waves in magnetic and rotating stars (Campos, 2011)

Details MAG waves in magnetic and rotating stars (Campos, 2011) MAG waves in magnetic and rotating stars (Campos, 2011)

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..74100735c&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/410/735. Originally published in: 2011MNRAS.410..735C

Computer Science

Stars: Nearby, Magnetic Fields

Scientific paper

The expression for the energy flux of magnetoacoustic-gravity-inertial (MAGI) waves derived in the Part I (Campos, 2011MNRAS.410..717C) of the present paper is applied to the luminosity of stars, leading to more than 60 relations between observable stellar quantities. Three of these relations are compared with empirical data, viz. concerning stellar luminosity or brightness compared with (i) magnetic field strength for strong magnetic stars, (ii) rotation period for fast rotating stars and (iii) mass and temperature for stars in general.
(4 data files).

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