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The ultraviolet spectrum of HH 24A and its relation to optical spectraThe spectrum of the brightest part (HH 24A) of the complex Herbig-Haro object HH 24 in the short wavelength UV range was studied. The object is of special interest since it is known that in the optical range the continuum is due to dust scattered light originating in a young stellar object while the shock excited emission lines are formed in HH 24A itself. The spectrum shows only a continuum or a quasi-continuum and is not comparable to that of the typical high excitation object like HH1 or HH2 nor to that of a low excitation object like HH3 or HH47.
Document ID
19910018737
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Boehm, K. H. (Washington Univ. Seattle., United States)
Noriega-Crespo, A. (Washington Univ. Seattle., United States)
Solf, J. (Max-Planck-Inst. fuer Astronomie Heidelberg (Germany, F.R.)., United States)
Brugel, E. W. (Colorado Univ. Boulder., United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1991
Subject Category
Astronomy
Report/Patent Number
NAS 1.26:188649
NASA-CR-188649
Accession Number
91N28051
Funding Number(s)
CONTRACT_GRANT: NAG5-45
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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