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The ultraviolet spectrum of the high redshift BL lac object 0215+015The highly variable object 0215+015 is studied. It has a range in the optical band of more than 4 magnitudes, and exhibits radidly variable polarization. At optical wavelengths it shows no emission lines but has a rich absorption spectrum with at least six, separate redshift systems. Combined are 3 LWP low-dispersion images of the object to produce a high signal-to-noise spectrum between 2400 - 3200 A which is use to study the hydrogen Lyman lines of the various redshift systems.
Document ID
19820023310
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Blades, J. C.
(Science Research Council Slough, United Kingdom)
Pettini, M.
(Royal Greenwich Observatory)
Hunstead, R. W.
(Sydney Univ.)
Murdoch, H. S.
(Sydney Univ.)
Date Acquired
August 10, 2013
Publication Date
January 1, 1982
Publication Information
Publication: NASA. Goddard Space Flight Center Advan. in Ultraviolet Astron.
Subject Category
Astronomy
Accession Number
82N31186
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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