B fields in OB stars (BOB): on the detection of weak magnetic fields in the two early B-type stars β CMa and ϵ CMa - Possible lack of a “magnetic desert” in massive stars

L. Fossati; N. Castro; T. Morel; N. Langer; M. Briquet; T. A. Carroll; S. Hubrig; M. F. Nieva; L. M. Oskinova; N. Przybilla; F. R. N. Schneider; M. Schöller; S. Simón-Díaz; I. Ilyin; A. de Koter; A. Reisenegger; H. Sana

doi:10.1051/0004-6361/201424986

Home

All issues

Volume 574 (February 2015)

A&A, 574 (2015) A20

Full HTML

Free Access

Fig. 8

Open with DEXTER Download original image

Phase plot of the ⟨ B_z ⟩ values obtained for β CMa from the HARPS data and the best fitting sine wave function. The symbols are as in the top left panel of Fig. 6.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.