Rotational studies of late-type stars. III - Rotation among BY Draconis stars

Details Rotational studies of late-type stars. III - Rotation among BY Draconis stars Rotational studies of late-type stars. III - Rotation among BY Draconis stars

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...269..250v&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 269, June 1, 1983, p. 250-252.

Other

63

Binary Stars, Dwarf Stars, Late Stars, Stellar Rotation, Barium, High Resolution, K Stars, Line Spectra

Scientific paper

High-resolution line profiles have been obtained and v sin i's measured
for 17 K and M dwarfs. All BY Draconis stars (whether single or in
binaries) rotate more rapidly than other K and M dwarfs, reinforcing
previous suggestions that rapid rotation (≥5 km s-1) is
the underlying cause of the BY Draconis syndrome.

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