Methods and results for detecting magnetic fields on late-type stars.
暂无分享,去创建一个
[1] S. Baliunas,et al. Ultraviolet and optical spectrum studies of Lambda Andromedae - Evidence for atmospheric inhomogeneities , 1982 .
[2] R. Becker,et al. Two-component X-ray emission from RS Canum Venaticorum binaries , 1981 .
[3] G. Marcy. The magnetic field on the late-type dwarf XI Bootis A , 1981 .
[4] Jr. Robinson. Magnetic field measurements on stellar sources - A new method , 1980 .
[5] R. Rosner,et al. Magnetic fields and coronal heating , 1980 .
[6] S. P. Worden,et al. Observations of magnetic fields on two late-type dwarf stars , 1980 .
[7] W. Cash,et al. X-rays from RS Canum Venaticorum systems - A HEAO 1 survey and the development of a coronal model , 1980 .
[8] D. S. Hall,et al. Starspots as the cause of the intrinsic light variations in RS Canum Venaticorum type stars , 1979 .
[9] R. Rosner,et al. Dynamics of the quiescent solar corona , 1978 .
[10] K. Eriksson,et al. Grid of model atmospheres for metal-deficient giant stars. I , 1975 .
[11] A. Title,et al. Measurements of solar magnetic fields by Fourier transform techniques , 1975 .
[12] H. W. Babcock. Magnetic Intensification of Stellar Absorption Lines. , 1949 .