High Rydberg state carbon recombination lines toward Cassiopeia A: 332 MHz VLA observations and comparison with H I and molecular lines

Details High Rydberg state carbon recombination lines toward Cassiopeia A: 332 MHz VLA observations and comparison with H I and molecular lines High Rydberg state carbon recombination lines toward Cassiopeia A: 332 MHz VLA observations and comparison with H I and molecular lines

Aug 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...430..682a&link_type=abstract

The Astrophysical Journal, vol. 430, no. 2, pt. 1, p. 682-689

Astronomy and Astrophysics

Astrophysics

20

Abundance, Cassiopeia A, H I Regions, Hydrogen, Interstellar Matter, Radio Emission, Rydberg Series, Astronomical Models, Cosmology, Neutral Gases, Recombination Reactions, Spectrum Analysis, Very Large Array (Vla)

Scientific paper

We present observations of the C270 alpha carbon recombination line, 21 cm neutral hydrogen line and (12)CO (J = 1 right arrow 0) molecular line toward Cas A. A comparison of the distribution of recombination line optical depths over the face of Cas A with that of H I optical depths and molecular line emission favors the association of C270 alpha regions with H I rather than molecular clouds. The association makes it possible to self-consistently determine several physical parameters of the clouds by combining the recombination line and 21 cm H I measurements.

Affiliated with

Also associated with

No associations

Rating

High Rydberg state carbon recombination lines toward Cassiopeia A: 332 MHz VLA observations and comparison with H I and molecular lines 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 High Rydberg state carbon recombination lines toward Cassiopeia A: 332 MHz VLA observations and comparison with H I and molecular lines, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High Rydberg state carbon recombination lines toward Cassiopeia A: 332 MHz VLA observations and comparison with H I and molecular lines will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1494204