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dc.contributor.authorFoltz, C. B.
dc.contributor.authorWilkes, Belinda Jane
dc.contributor.authorPeterson, B. M.
dc.date.accessioned2017-06-08T20:40:35Z
dc.date.issued1983
dc.identifierQuick submit: 2017-02-08T10:55:19-0500
dc.identifier.citationFoltz, C. B., B. J. Wilkes, and B. M. Peterson. 1983. “The H-Beta Emission Line Profile of Arakelian 120.” The Astronomical Journal 88 (December): 1702. doi:10.1086/113462.en_US
dc.identifier.issn0004-6256en_US
dc.identifier.urihttp://nrs.harvard.edu/urn-3:HUL.InstRepos:32955258
dc.description.abstractA high-quality (S/N in the range from 30 to 100), high-resolution (approximately 1.8 A) spectrum of the photometrically and spectroscopically variable Seyfert 1 galaxy Arakelian 120 has been obtained in the wavelength region including H-beta. The observed H-beta 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-beta is discussed.en_US
dc.description.sponsorshipAstronomyen_US
dc.language.isoen_USen_US
dc.publisherIOP Publishingen_US
dc.relation.isversionof10.1086/113462en_US
dash.licenseLAA
dc.titleThe H-beta emission line profile of Arakelian 120en_US
dc.typeJournal Articleen_US
dc.date.updated2017-02-08T15:55:21Z
dc.description.versionVersion of Recorden_US
dc.relation.journalThe Astronomical Journalen_US
dash.depositing.authorWilkes, Belinda Jane
dc.date.available1983
dc.date.available2017-06-08T20:40:35Z
dc.identifier.doi10.1086/113462*
dash.contributor.affiliatedWilkes, Belinda


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