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The L-alpha/H-alpha intensity ratio in PKS 0237-23The ratio I(L-alpha)/I(H-alpha) has been measured to be 1.7 plus or minus 0.6 in the quasar PKS 0237-23. The measured ratio is similar to that measured in 3C 273 by Davidsen et al. and to that inferred by Baldwin from a study of a large number of quasars; it is a factor of 5 to 14 smaller than expected from recombination theory. If the L-alpha radiation is resonantly scattered and there are modest amounts of dust within the ionized region, the measured ratio may be interpreted in terms of recombination theory, with L-alpha being depleted by absorption by the dust.
Document ID
19780044083
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Hyland, A. R.
(Hale Observatories Pasadena, CA, United States)
Becklin, E. E.
(Hale Observatories Pasadena, CA, United States)
Neugebauer, G.
(Hale Observatories Pasadena, Calif., United States)
Date Acquired
August 9, 2013
Publication Date
March 15, 1978
Publication Information
Publication: Astrophysical Journal
Subject Category
Astronomy
Accession Number
78A27992
Funding Number(s)
CONTRACT_GRANT: NSF AST-74-18555-A2
CONTRACT_GRANT: NGL-05-002-207
Distribution Limits
Public
Copyright
Other

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