Profile variability of the H$\mathsf{\alpha}$ and H$\mathsf{\beta}$ broad emission lines in NGC 5548-Reference-Cited by-同舟云学术

Profile variability of the H$\mathsf{\alpha}$ and H$\mathsf{\beta}$ broad emission lines in NGC 5548

Published:2004-07-16 Issue:3 Volume:422 Page:925-940
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Shapovalova A. I.,Doroshenko V. T.,Bochkarev N. G.,Burenkov A. N.,Carrasco L.,Chavushyan V. H.,Collin S.,Valdés J. R.,Borisov N.,Dumont A.-M.,Vlasuyk V. V.,Chilingarian I.,Fioktistova I. S.,Martinez O. M.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:20035652/pdf

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3. Begelman, M. C. 1985, in Astrophysics of Active Galaxies and Quasi-Stellar Objects, ed. J. S. Miller (Mill Valley, CA: Univ. Sci.), 411

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