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Publication year - 1976

Publication title -

astronomische nachrichten

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 0.394

H-Index - 63

eISSN - 1521-3994

pISSN - 0004-6337

DOI - 10.1002/asna.19762970507

Subject(s) - equator , physics , spots , stars , magnetic field , magnetic dip , rotation (mathematics) , astrophysics , latitude , field strength , field (mathematics) , l shell , astronomy , geometry , chemistry , earth's magnetic field , mathematics , quantum mechanics , pure mathematics

It is concluded that the generation regions of the spots are disposed in latitudes below 60° relative to the rotation equator in Ap stars. The strongest Sr spots coincide with the extremes of the magnetic field in 17 Com A whereas the number of spots is correlated with the strength of the magnetic field. For β CrB a correlation is found between the strength of the magnetic field deduced from different Fe I lines and the effective optical depth at which these lines are formed.

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