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The structure of Herbig-Haro object 43 and Orion dark cloud extinctionNew ultraviolet and optical observations of Herbig-Haro Object No. 43 are reported. Continuum and emission line fluxes in the range 1250 A equal to or less than lambda equal to less than 7350A have been measured. The continuum fluxes are best matched by an enhanced H two photon component added to H free bound emission, assuming theta Ori extinction curve with E(B-V) = 0.2, R = 5. The strucutre and dynamics of three components within the object are discussed. The object has a radiative output of equal to or greater than 0.23 infrared luminosity in ultraviolet and optical radiation combined. The energy requirements are discussed in terms of the production of shock waves by a collimated, supersonic mass outflow from a nearby infrared source.
Document ID
19850027518
Acquisition Source
Legacy CDMS
Document Type
Technical Memorandum (TM)
Authors
Schwartz, R. D.
(Missouri Univ. St. Louis, United States)
Dopita, M. A.
(Australian National Univ. Moffett Field, CA, United States)
Cohen, M.
(NASA Ames Research Center)
Date Acquired
September 5, 2013
Publication Date
January 1, 1984
Subject Category
Astronomy
Report/Patent Number
NAS 1.15:87503
NASA-TM-87503
Accession Number
85N35831
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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