A note on the relation between magnetic fields and the 5200 A feature in helium-weak stars

Details A note on the relation between magnetic fields and the 5200 A feature in helium-weak stars A note on the relation between magnetic fields and the 5200 A feature in helium-weak stars

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...138..493m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 138, no. 2, Sept. 1984, p. 493, 494.

Astronomy and Astrophysics

Astrophysics

9

Magnetic Stars, Peculiar Stars, Stellar Composition, Stellar Magnetic Fields, Stellar Spectra, Correlation Coefficients, Hot Stars, Stellar Temperature

Scientific paper

Magnetic field strengths and the 5200 A feature appear to be correlated in He-weak stars. This is further evidence that they form the hot extension of the upper main sequence, chemically peculiar stars, both of their magnetic and nonmagnetic branches. To take account of this situation, an extension of Preston's (1974) nomenclature of CP-stars is suggested.

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