Interstellar CN rotational spectra: (12)C(15)N

Details Interstellar CN rotational spectra: (12)C(15)N Interstellar CN rotational spectra: (12)C(15)N

Nov 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...436..176s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-367X), vol. 436, no. 1, p. 176-182

Astronomy and Astrophysics

Astrophysics

5

Astronomical Observatories, Cyanides, Diatomic Molecules, Rotational Spectra, Galaxies, Infrared Spectra, Mathematical Models

Scientific paper

We confirm the earlier KOSMA 3 m radiotelescope detection of (12)C(15)N (N = 2 goes to 1) in Orion A (Saleck et al. 1993) by follow-up measurements of the strongest components of two rotational stransitions, N = 1 goes to 0 and N = 2 goes to 1 with the IRAM 30 m telescope. The newly obtained and highly precise data are used together with laboratory data on (12)C(14)N and C-13N-14 reported in the literature to reveal a deviation of the Born-NO. Furthermore, the (12)C(14)N rotational spectrum is predicted up to 1 THz.

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