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Interstellar lines other than hydrogen

Published online by Cambridge University Press:  14 August 2015

G.H. Herbig
G.H. Herbig*
Affiliation:
Lick Observatory, University of California, Santa Cruz, Calif., U.S.A.

Extract

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I would like to extrapolate beyond the present state of interstellar line spectroscopy toward the next generation of satellite-borne equipment, but with due recognition of the fact that more work still has to be done from the Earth's surface.

Type
Part III: Interstellar Absorption and Emission
Information
Symposium - International Astronomical Union , Volume 36: Ultraviolet Stellar Spectra and Related Ground-Based Observations , 1970 , pp. 315 - 319
Copyright
Copyright © Reidel 1970 

References

Borgström, A.: 1968, Ark. Fys. 38, 243.Google Scholar
Herbig, G. H.: 1968, Z. Astrophys. 68, 243.Google Scholar
Herbig, G. H.: 1969, ‘Pre-Main Sequence Stellar Evolution’, Mem. Soc. Roy. Sci. Liège (in press).Google Scholar
Hobbs, L. M.: 1969, Astrophys. J. 157, 135.CrossRefGoogle Scholar
Larimer, J. W.: 1967, Geochim. Cosmochim. Acta 31, 1215.Google Scholar
Spite, M.: 1968, Ann. Astrophys. 31, 269.Google Scholar