The Origin of c2 in Comets CYCLE4MEDIUM

Details The Origin of c2 in Comets CYCLE4MEDIUM The Origin of c2 in Comets CYCLE4MEDIUM

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994hst..prop.5462a&link_type=abstract

HST Proposal ID #5462

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Hst Proposal Id #5462 Solar System Comets

Scientific paper

We propose to observe any comet which satisfies the constraint Q(C2) > 1.4E26 at r=1AU (scaled appropriately to other r) to map the Mulliken and Swan bands of C2. The relative intensities of the singlets and triplets and the excitation temperatures will be mapped as a function of distance from the nucleus. This will constrain the presently unknown formation mechanism for producing C2 and thus constrain the identity of its parent. It will also constrain the rate for intercombination (singlet-triplet) radiative transitions, thus providing crucial information required for the detailed study of the resonance fluorescence of C2.

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