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Two Multifrequency Observations of 3C 371

Worrall, D. M. and Puschell, J. J. and Bruhweiler, F. C. and Miller, H. R. and Rudy, R. J. and Ku, W. H. M. and Aller, M. F. and Aller, H. D. and Hodge, P. E. and Matthews, K. and Neugebauer, G. and Soifer, B. T. and Webb, J. R. and Pica, A. J. and Pollock, J. T. and Smith, A. G. and Leacock, R. J. (1984) Two Multifrequency Observations of 3C 371. Astrophysical Journal, 278 . pp. 521-529. ISSN 1538-4357. http://resolver.caltech.edu/CaltechAUTHORS:20170307-150414789

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Abstract

We present observations of 3C 371, made at frequencies from the radio to the ultraviolet, which were coordinated during two short time intervals separated by 3 months. We also present 1 keV X-ray flux densities measured at a different time. The multifrequency measurements indicate spectral steepening at visual wavelengths, and that an extrapolation of the ultraviolet continuum falls below the X-ray data. We explain the infrared through X-ray data as relativistically beamed synchrotron self-Compton emission and derive source parameters for two possible models. Our ultraviolet spectra both show strong Lyɑ emission at the same redshift as weak optical emission lines reported previously. We favor production of these lines by recombination of gas after its ionization by the ultraviolet to X-ray continuum radiation. We tentatively identify C IV and N v absorption lines in one of our ultraviolet spectra, which, if real, suggest the presence of a hot (~ 3 x 10^5 K) gaseous halo in 3C 371.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1086/161818DOIArticle
http://adsabs.harvard.edu/abs/1984ApJ...278..521WADSArticle
Additional Information:© 1984 American Astronomical Society. Received 1983 June 9; accepted 1983 August 30. We thank Professor M. J. Rees and Dr. R. C. Puetter for enlightening discussions. Drs. P. Le Van, R. Puetter, and H. E. Smith are thanked for their assistance in the acquisition of the infrared data. We thank the IVE observatory staff for assistance in obtaining and reducing the IVE observations, particularly Dr. D. Klinglesmith for making available the Fahey-Klinglesmith software package. The IVE work was supported by NASA grant NAG 5-63, the Michigan radio astronomy by NSF grant AST 80-21250, the KPNO observations by the US Air Force Office of Scientific Research grant 81-0161, the Rosemary Hill Observatory measurements by NSF grant AST-8203926, the Caltech measurements by an NSF grant, and the Einstein Observatory work by NASA grant NAS-8-30753.
Funders:
Funding AgencyGrant Number
NASANAG 5-63
NSFAST-8021250
Air Force Office of Scientific Research (AFOSR)81-0161
NSFAST-8203926
NASANAS-8-30753
Subject Keywords:BL Lacertae objects galaxies: individual radio sources: galaxies ultraviolet: spectra X-rays: sources
Record Number:CaltechAUTHORS:20170307-150414789
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20170307-150414789
Official Citation:Two multifrequency observations of 3C 371 Worrall, D. M., Puschell, J. J., Miller, H. R., Rudy, R. J., Ku, W. H.-M., Aller, M. F., , Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 278, March 15, 1984, p. 521-529.
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:74870
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:07 Mar 2017 23:26
Last Modified:07 Mar 2017 23:26

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