Spectroscopic changes of the magnetic CP star γ Equulei.

Details Spectroscopic changes of the magnetic CP star γ Equulei. Spectroscopic changes of the magnetic CP star γ Equulei.

Sep 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26a...325..529s&link_type=abstract

Astronomy and Astrophysics, v.325, p.529-534

Astronomy and Astrophysics

Astrophysics

14

Stars: Chemically Peculiar, Stars: Individual: {Gamma} Equ, Stars: Magnetic Fields, Stars: Rotation

Scientific paper

From an analysis of some new spectroscopic observations of the magnetic CP star γ Equ we derived an effective magnetic field of -930+/-150G and a surface magnetic field of 4000G. The magnitude of the effective field is compatible with a variation of the field on a time scale of a little more than 70 years. The temporal behaviour of the magnetic field is explained by the superposition of a dipole and quadrupole and the model of the oblique rotator. Surprisingly a few radial velocity values differ from the expected ones by about 10km/s.

Affiliated with

Also associated with

No associations

Rating

Spectroscopic changes of the magnetic CP star γ Equulei. 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 Spectroscopic changes of the magnetic CP star γ Equulei., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectroscopic changes of the magnetic CP star γ Equulei. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1222435