Detection of HC11N in the cold dust cloud TMC-1

Details Detection of HC11N in the cold dust cloud TMC-1 Detection of HC11N in the cold dust cloud TMC-1

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...291l..63b&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 291, April 15, 1985, p. L63-L65.

Astronomy and Astrophysics

Astrophysics

25

Astronomical Spectroscopy, Hydrocyanic Acid, Molecular Clouds, Molecular Rotation, Spectral Line Width

Scientific paper

The authors report the detection of the J = 41→40 rotational transition of HC11N in the direction of the Taurus molecular cloud complex. The line strength is in good agreement with predicted values, and the rotational parameters, although determined more accurately with these results, remain unchanged from those obtained previously using observations of IRC +10°216 alone.

Affiliated with

Also associated with

No associations

Rating

Detection of HC11N in the cold dust cloud TMC-1 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 Detection of HC11N in the cold dust cloud TMC-1, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Detection of HC11N in the cold dust cloud TMC-1 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1288799