The 3.4 micron emission in comets.

Details The 3.4 micron emission in comets. The 3.4 micron emission in comets.

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989iaus..135p.431b&link_type=abstract

IAU Symposium No. 135: Interstellar dust: contributed papers, p. 431

Physics

Comets: Infrared Radiation, Comet 1987 Xxix Bradfield, Comet 1986 Iii Halley

Scientific paper

Emission features near 3.4 μm were detected in comet Bradfield (1987s) on 17 Nov. 1987 UT, and, marginally, on two earlier dates, with the Cooled Grating Array Spectrometer at the NASA IRTF. The central wavelength (3.36 μm) and width (≡0.15 μm) of the strongest feature coincide with those observed in comet Halley. A weaker emission feature at 3.52 μm and a strong feature extending shortward of 2.9 μm were also detected. This brings the number of comets in which these three features have been seen to three, two new (Bradfield, Wilson) and one old (Halley).

Affiliated with

Also associated with

No associations

Rating

The 3.4 micron emission in comets. 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 The 3.4 micron emission in comets., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The 3.4 micron emission in comets. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1571409