The interpretation of the 3.2-3.5 micron emission feature in the spectrum of Comet P/Halley - Abundances in the comet and in interstellar matter
T. Encrenaz(Centre National de la Recherche Scientifique), J.‐L. Puget(Université Paris-Sud), L. D’Hendecourt
Unknown
December 1, 1988
Cited by 21
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