Detection of the N = 1 - 0 transition of C4H

Details Detection of the N = 1 - 0 transition of C4H Detection of the N = 1 - 0 transition of C4H

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...255l..75b&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 255, Apr. 1, 1982, p. L75-L79.

Astronomy and Astrophysics

Astrophysics

15

Butenes, Electron Transitions, Hyperfine Structure, Interstellar Chemistry, Molecular Clouds, Molecular Rotation, Carbon Stars, Electron Spin, Normal Density Functions, Spectral Resolution, Stellar Spectra

Scientific paper

Five hyperfine components of the N = 1 - 0 rotational transition of C4H have been detected toward the dust cloud TMC-1. Using these and previously published data, rotation, spin-rotation, and hyperfine constants have been determined for the molecule. An upper limit is presented for the intensity of the strongest component in IRC + 10 deg 216.

Affiliated with

Also associated with

No associations

Rating

Detection of the N = 1 - 0 transition of C4H 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 the N = 1 - 0 transition of C4H, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Detection of the N = 1 - 0 transition of C4H will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-840849