The magnetic field of pulsating stars

Details The magnetic field of pulsating stars The magnetic field of pulsating stars

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15.1016a&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, Nov. 1989, p. 1016-1019. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Stellar Magnetic Fields, Stellar Oscillations, Variable Stars, Amplitude Distribution Analysis, Magnetic Flux, Pulsars, Radial Velocity

Scientific paper

The physical values determining variations in magnetic field intensity in pulsating stars are analyzed to obtain a constant R describing the relations between the amplitude of magnetic field intensity, semiamplitude of radial velocity variation, and the effective temperature of the envelope. Calculations for several types of pulsating stars are performed to validate the constant. The formula is used to estimate the probable amplitude of the field intensity variation of a star from values for the semiamplitude of radial velocity variation and the effective temperature of the envelope.

Affiliated with

Also associated with

No associations

Rating

The magnetic field of pulsating stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The magnetic field of pulsating stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The magnetic field of pulsating stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1617404