Spectroscopic study of the Am SB2 eclipsing binary HR 6611

Details Spectroscopic study of the Am SB2 eclipsing binary HR 6611 Spectroscopic study of the Am SB2 eclipsing binary HR 6611

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004mast.conf..191m&link_type=abstract

Magnetic stars, Proceedings of the International Conference, held in the Special Astrophysical Observatory of the Russian AS, Au

Astronomy and Astrophysics

Astrophysics

3

Binaries, Eclipsing, Hr 6611, Abundances, Magnetic Fields

Scientific paper

Detailed spectroscopic study confirmed a mild Am-peculiarity of both components of the double-lined spectroscopic eclipsing binary HR 6611 and revealed a slightly asynchronous rotation of the primary one. The analysis of Zeeman spectra of the binary and 4 non-magnetic stars, does not exclude an effective magnetic field on HR 6611A, varying cyclically with a semi-amplitude of 0.2 kG, but definitely not with the orbital period 3.895 d.

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