Carbon production in comet West 1975n

Details Carbon production in comet West 1975n Carbon production in comet West 1975n

Oct 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...209l..45f&link_type=abstract

Astrophysical Journal, vol. 209, Oct. 1, 1976, pt. 2, p. L45-L48.

Computer Science

Sound

91

Abundance, Carbon, Comet Heads, Emission Spectra, Rocket Sounding, Ultraviolet Spectra, Aerobee Rocket Vehicle, Carbon Monoxide, Hydroxyl Emission, Metastable State, Photodissociation, Ultraviolet Spectrophotometers, Water Vapor

Scientific paper

Rocket-ultraviolet spectra of comet West 1975n are reported which were obtained with scanning spectrophotometers in the wavelength range from 1200 to 1300 A. The principal emission features observed include lines of C, O, and C(+), as well as bands of OH, CO, CO(+). The estimated fluxes of the C, O, H, CO, and OH features are found to be consistent with a photodissociation source in which the CO evaporation rate is about one-third that of water. The presence of a large number of carbon atoms in the metastable 1D state is indicated and taken to suggest that dissociative recombination is important near the cometary nucleus, that CO must originate in the nucleus, and that CO is the primary carbon constituent of the comet.

Affiliated with

Also associated with

No associations

Rating

Carbon production in comet West 1975n does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Carbon production in comet West 1975n, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Carbon production in comet West 1975n will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1568005