A high-velocity magnetic degenerate, G35-26

Details A high-velocity magnetic degenerate, G35-26 A high-velocity magnetic degenerate, G35-26

Jun 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978pasp...90..303g&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 90, June-July 1978, p. 303-306.

Astronomy and Astrophysics

Astronomy

10

Magnetic Stars, Stellar Magnetic Fields, Stellar Spectra, Zeeman Effect, Abundance, Stellar Models, Stellar Motions

Scientific paper

This proper-motion star (Gr 469) has a predicted absolute visual magnitude of +11.4 and the high tangential velocity of 263 km/s. It shows both hydrogen and helium absorption lines well-represented by a field of 8 megagauss. The temperature is 16,000 K, and the radius normal. The resolved H-beta Zeeman components are abnormally sharp; a not completely explained feature exists at 5050 A. It is suggested that about half the known degenerates with resolved Zeeman components have both hydrogen and helium in their atmospheres.

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