Spectrophotometric observations of Comet Austin (1982g)

Y. Mekler; M. Podolak

doi:10.1007/BF00054332

Spectrophotometric observations of Comet Austin (1982g)

Y. Mekler^*, M. Podolak

^*Corresponding author for this work

Department of Geophysics

Research output: Contribution to journal › Article › peer-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 language	English
Pages (from-to)	39-46
Number of pages	8
Journal	Earth, Moon and Planets
Volume	44
Issue number	1
DOIs	https://doi.org/10.1007/BF00054332
State	Published - Jan 1989

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10.1007/BF00054332

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title = "Spectrophotometric observations of Comet Austin (1982g)",

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.",

author = "Y. Mekler and M. Podolak",

year = "1989",

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AB - 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.

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JO - Earth, Moon and Planets

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Spectrophotometric observations of Comet Austin (1982g)

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