Abstract
view Abstract Citations (73) References (10) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Rotational studies of late-type stars. III. Rotation among BY Draconis stars. Vogt, S. S. ; Soderblom, D. R. ; Penrod, G. D. Abstract 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. Publication: The Astrophysical Journal Pub Date: June 1983 DOI: 10.1086/161035 Bibcode: 1983ApJ...269..250V Keywords: Binary Stars; Dwarf Stars; Late Stars; Stellar Rotation; Barium; High Resolution; K Stars; Line Spectra; Astrophysics full text sources ADS | data products SIMBAD (16) Related Materials (6) Part 1: 1982ApJ...263..239S Part 2: 1983ApJS...53....1S Part 4: 1993ApJS...85..315S Part 5: 1993ApJ...402L...5S Part 6: 1998Ap&SS.261...59S Part 7: 2001ApJ...563..334S
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