The H-beta emission line profile of Arakelian 120 | Zendy

C. B. Foltz | Zendy; B. J. Wilkes | Zendy; B. M. Peterson | Zendy

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The H-beta emission line profile of Arakelian 120

Author(s) -

C. B. Foltz,

B. J. Wilkes,

B. M. Peterson

Publication year - 1983

Publication title -

the astronomical journal

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.61

H-Index - 271

eISSN - 1538-3881

pISSN - 0004-6256

DOI - 10.1086/113462

Subject(s) - physics , emission spectrum , beta (programming language) , astrophysics , line (geometry) , astronomy , spectral line , geometry , mathematics , computer science , programming language

A high-quality (30 < S/N < 100), high-resolution (~ 1.8 Á) spectrum of the photometrically and spectroscopically variable Seyfert 1 galaxy Arakelian 120 has been obtained in the wavelength region including H# The observed Hji? line profile can be considered as a benchmark for future line profile studies of this interesting object. The origin of the extended red wing of H/? is discussed.

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