Hydrogen lines Stark broadening tables in the presence of a magnetic field

Details Hydrogen lines Stark broadening tables in the presence of a magnetic field Hydrogen lines Stark broadening tables in the presence of a magnetic field

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26as...59..229m&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 59, Feb. 1985, p. 229-253. Research supported by the Max-Pla

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Astronomical Catalogs, Hydrogen, Lyman Alpha Radiation, Spectral Line Width, Stark Effect, Stellar Magnetic Fields, Computational Astrophysics, Electron Density (Concentration), H Alpha Line, Line Shape, Lyman Beta Radiation, Stellar Temperature

Scientific paper

Tables of Stark broadened profiles of the lines Lα, Lβ and Hα of hydrogen, in the presence of a magnetic field are presented. Unpolarized intensities observed in directions parallel (longitudinal profiles) and perpendicular (transversal profiles) to the magnetic field have been computed on the basis of the unified theory, for electron densities higher than or equal to 1015cm-3, temperatures ranging from 5×103 to 4×104K, and magnetic fields up to 4×104G.

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