Evidence for a radial magnetic field gradient on the AP star Alpha(2) Canum Venaticorum

Details Evidence for a radial magnetic field gradient on the AP star Alpha(2) Canum Venaticorum Evidence for a radial magnetic field gradient on the AP star Alpha(2) Canum Venaticorum

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pazh...10..443r&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 10, June 1984, p. 443-448) Soviet Astronomy Letters (ISSN 0360-0327), vol. 10, May-June

Astronomy and Astrophysics

Astronomy

7

A Stars, Line Spectra, Magnetic Field Configurations, Peculiar Stars, Stellar Magnetic Fields, B Stars, Balmer Series, Zeeman Effect

Scientific paper

The investigation of the Ap star α2 CVn showed a
decrease of the value and amplitude of variation of the magnetic field
measured from the lines shorter than 3646 Å in comparison with the
measurements at longer wavelengths. For another Ap star, β CrB, no
such effect was observed.

Affiliated with

Also associated with

No associations

Rating

Evidence for a radial magnetic field gradient on the AP star Alpha(2) Canum Venaticorum 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 Evidence for a radial magnetic field gradient on the AP star Alpha(2) Canum Venaticorum, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evidence for a radial magnetic field gradient on the AP star Alpha(2) Canum Venaticorum will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1855740