Cosmic Background Radiation Temperature from CN Absorption
Abstract
Precise high-resolution measurements of the interstellar lines of CN near 3874 A toward the star Zeta Oph provide a new measurement of the cosmic background radiation temperature of 2.74 + or - 0.05 K at 2.64 mm and 2.75 (+0.24, -0.29) K at 1.32 mm. Using a spectral resolution of 156,000, the intrinsic width of these lines is found to be 19.0 + or - 0.5 mA, which is substantially smaller than previously reported and requires larger saturation corrections than used in previous work to determine the CN excitation temperature.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- October 1986
- DOI:
- 10.1086/164650
- Bibcode:
- 1986ApJ...309..822C
- Keywords:
-
- Cosmic Noise;
- Cyanogen;
- Galactic Radiation;
- Stellar Spectra;
- Background Radiation;
- Line Spectra;
- Ophiuchi Clouds;
- Spectral Resolution;
- Astrophysics;
- COSMIC BACKGROUND RADIATION;
- COSMOLOGY;
- INTERSTELLAR: MOLECULES;
- LINE PROFILES