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- W2007168538 abstract "view Abstract Citations (176) References (19) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The Mean Surface Fields of Magnetic Stars Preston, George W. Abstract Estimates of mean surface fields H, for twenty-eight Ap stars of the Sr-Cr-Eu class with V sin i < 10 km have been obtained from measurements of magnetically resolved or broadened absorption lines. The fields so obtained do not appear to be correlated with UB V color indices, Eu ii line strengths, or rotational velocities inferred from periods for this group of stars. The frequency distribution of H, is characterized by a maximum between 2 and 3 kilogauss and a tail that extends beyond 10 kilogauss. Indirect arguments based on effective magnetic fields suggest that mean surface fields may increase systematically with rotational velocity, but observational bias and certain selection effects render this conclusion suspect. Publication: The Astrophysical Journal Pub Date: March 1971 DOI: 10.1086/150840 Bibcode: 1971ApJ...164..309P full text sources ADS | data products SIMBAD (44)" @default.
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- W2007168538 title "The Mean Surface Fields of Magnetic Stars" @default.
- W2007168538 doi "https://doi.org/10.1086/150840" @default.
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