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The Gum nebulaThe distance from the sun to the center of the star, Gamma Velorium, is determined in an effort to draw a physical model and identify the ionized energy source of the Gum nebula. The distance is calculated from the local hydrogen density of radio astronomy studies and the hydrogen measure.
Document ID
19720015710
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Brandt, J. C. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 6, 2013
Publication Date
January 1, 1972
Publication Information
Publication: Significant Accomplishments in Sci., 1970
Subject Category
Space Sciences
Accession Number
72N23360
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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IDRelationTitle19720015674Collected WorksSignificant Accomplishments in Sciences, 1970N72-23324 14-13Collected Works
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