Radio recombination lines of carbon as a tool for investigation of molecular clouds
Author:
Publisher
Informa UK Limited
Subject
Astronomy and Astrophysics,Instrumentation
Link
http://www.tandfonline.com/doi/pdf/10.1080/10556799608205467
Reference33 articles.
1. Ionized gas towards galactic centre — Constraints from low-frequency recombination lines
2. Detection of carbon recombination lines below 100 MHz towards the Galactic Centre and M16
3. High Rydberg state carbon recombination lines toward Cassiopeia A: 332 MHz VLA observations and comparison with H I and molecular lines
4. VLA observations of 21 centimeter H I absorption toward Cassiopeia A
5. Identification of the anomalous 26.131-MHz nitrogen line observed towards Cas A
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1. OBSERVATIONS OF DECAMETER CARBON RADIO RECOMBINATION LINES IN SEVERAL GALACTIC DIRECTIONS Part 2. ANALYSIS OF PHYSICAL CONDITIONS IN DIFFUSE CII REGIONS;RADIO PHYSICS AND RADIO ASTRONOMY;2023
2. A high-resolution study of carbon radio recombination lines towards Cassiopeia A;Monthly Notices of the Royal Astronomical Society;2019-03-16
3. Detection and application of carbon recombination lines in millimeter range;Kinematics and Physics of Celestial Bodies;2010-08
4. Carbon recombination lines from the Galactic plane at 34.5 & 328 MHz;Journal of Astrophysics and Astronomy;2001-03
5. Physical conditions in photodissociation regions from observations of carbon radio recombination lines and IR fine-structure lines of CII and OI;Astronomy Reports;2000-07
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