Detection of interstellar methyldiacetylene (CH3C4H) in the dark dust cloud TMC 1

Details Detection of interstellar methyldiacetylene (CH3C4H) in the dark dust cloud TMC 1 Detection of interstellar methyldiacetylene (CH3C4H) in the dark dust cloud TMC 1

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...134l..11w&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 134, no. 2, May 1984, p. L11-L14. Sponsorship: Deutsche Forschungsgemeinschaft

Astronomy and Astrophysics

Astronomy

23

Acetylene, Cyano Compounds, Interstellar Chemistry, Methyl Compounds, Molecular Chains, Molecular Clouds, Abundance, Ammonia, Radio Sources (Astronomy), Radio Spectroscopy

Scientific paper

The K = 0 and K = 1 components of the J = 6 → 5 and 5 → 4 transitions of methyldiacetylene (CH3C4H) have been detected in the nearby dust cloud TMC1 using the Effelsberg 100-m telescope. The abundance of this species is comparable to that of the cyanopolyynes as well as to that of methylacetylene (CH3C2H). The authors have also found the (5,2) transition of NH3 towards the galactic center molecular cloud Sgr B2.

Affiliated with

Also associated with

No associations

Rating

Detection of interstellar methyldiacetylene (CH3C4H) in the dark 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 interstellar methyldiacetylene (CH3C4H) in the dark dust cloud TMC 1, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Detection of interstellar methyldiacetylene (CH3C4H) in the dark dust cloud TMC 1 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1367506