Spectrophotometric observations of Comet Austin (1982g)

Y. Mekler*, M. Podolak

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

Spectrophotometric observations of Comet Austin (1982g) in the bands of CN, C2, and C3 are presented, and fit to a Haser model for the cometary brightness distribution. The lifetimes of the parent and daughter molecules, as well as the velocity of the molecules leaving the cometary surface are determined from the model fit. The absolute production rate of molecules is also determined.

Original languageEnglish
Pages (from-to)39-46
Number of pages8
JournalEarth, Moon and Planets
Volume44
Issue number1
DOIs
StatePublished - Jan 1989

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