Interstellar C2 molecules toward OMI Persei.
Abstract
Seven weak interstellar absorption lines of the (2-0) Phillips band of C2 near the wavelength 8760 are detected in the spectrum of Omicron Persei. All of the lines have equivalent widths less than 2 mA and originate from the five lowest rotational levels of C2. The resulting total column density is N(C2) = 1.5 x 10 to the 13th/sq cm, and the excitation temperature is T = 116 plus or minus 16 K.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- January 1981
- DOI:
- Bibcode:
- 1981ApJ...243..485H
- Keywords:
-
- Absorption Spectra;
- Abundance;
- Carbon;
- Interstellar Matter;
- Stellar Spectra;
- Density (Mass/Volume);
- Spectral Line Width;
- Astrophysics