ASPCS
 
Back to Volume
Paper: Spatial Distribution of Early Spectral Type Magnetic Stars
Volume: 510, Stars: From Collapse to Collapse
Page: 270
Authors: Boronina, S. V.; Kholtygin, A. F.
Abstract: We have taken O, B, A and F magnetic stars from the catalog by Bychkov et. al (2009) and divided them into three groups: stars with the rms magnetic field strength ⟨B⟩e> 100G was accepted as "suspected to be magnetic". Some of the "suspected to be magnetic" stars satisfying both conditions ⟨B⟩e>2σ and χ2>1 were considered to be magnetic. The galactic coordinates and other parameters of all O, B, A, and F type stars were taken from SIMBAD. The spatial and surface densities of all considered types of stars were calculated.
eAccess Cost: $9.00
Back to Volume