Spatial distribution of magnetic CP stars (Kudryavtsev+, 2003)

Details Spatial distribution of magnetic CP stars (Kudryavtsev+, 2003) Spatial distribution of magnetic CP stars (Kudryavtsev+, 2003)

Nov 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ycatp016004602k&link_type=abstract

VizieR On-line Data Catalog: J/other/Ap/46.234. Originally published in: 2003Ap.....46..234K

Other

Stars: Peculiar, Magnetic Fields, Parallaxes: Trigonometric, Photometry: Ubv

Scientific paper

On the basis of analysis of original publications and our own measurements a Cataloque of magnetic chemically peculiar (CP) upper-main sequence stars has been established. The sample includes 211 magnetic CP stars with magnetic fields ranging from hundreds of gauss to dozens of kilogauss, for 49 of them the surface magnetic field (Be) has been measured from the Zeeman splitting.
The CP stars may be divided into 3 groups: reversing stars (table3, longitudinal field Be changes its sign), non-reversing (table4, Be keeps the same sign), and poorly studied stars.
(6 data files).

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