Chemical abundance of Hewk stars with weak and strong magnetic fields

Details Chemical abundance of Hewk stars with weak and strong magnetic fields Chemical abundance of Hewk stars with weak and strong magnetic fields

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007smma.conf...46g&link_type=abstract

Spectroscopic methods in modern astrophysics. Proceedings of the conference held 13-15 September 2006, Moscow, Russia. Eds. L. M

Astronomy and Astrophysics

Astrophysics

Scientific paper

This paper has as its objective of studying the properties of stars of different peculiarity with weak magnetic fields (Be<0.1kG) and their comparison with stars having strong magnetic fields (Be>3-5kG), in the given case - Hewk stars. In some of them the helium lines are invisible in the spectrum, although in normal stars of the same temperature they are at a disadvantage in intensity only to hydrogen lines. Stars with weak magnetic fields are poorly investigated because all researchers concentrated only on objects with strong magnetic fields.

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