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Ultraviolet continuum and H2 fluorescent emission in Herbig-Haro objects 43 and 47IUE short wavelength spectra are presented for the low excitation Herbig-Haro objects HH 43 and HH 47. In the former, several emission lines in the Lyman band of H2 from an excited state are observed which are due to fluorescence from the H Ly-alpha line pumping a lower state (that is in turn excited by a low-velocity shock wave). No evidence of highly ionized gas emission is found in the UV spectra, and both objects exhibit a UV continuum which peaks in the vicinity of 1500 A and is probably caused by H two-photon emission enhanced by low velocity shock collisional excitation.
Document ID
19830052013
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Schwartz, R. D.
(Missouri, University St. Louis, MO, United States)
Date Acquired
August 11, 2013
Publication Date
May 1, 1983
Publication Information
Publication: Astrophysical Journal, Part 2 - Letters to the Editor
Volume: 268
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
83A33231
Funding Number(s)
CONTRACT_GRANT: NAG5-243
CONTRACT_GRANT: NSF AST-82-01430
Distribution Limits
Public
Copyright
Other

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