Carbon Recombination Lines between 34.5 and 770 MHz toward Cassiopeia A
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/506/i=2/a=758/pdf
Reference38 articles.
1. High Rydberg state carbon recombination lines toward Cassiopeia A: 332 MHz VLA observations and comparison with H I and molecular lines
2. VLA observations of 21 centimeter H I absorption toward Cassiopeia A
3. Identification of the anomalous 26.131-MHz nitrogen line observed towards Cas A
4. Galactic hydrostatic equilibrium with magnetic tension and cosmic-ray diffusion
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