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| 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. |
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