High Rydberg state carbon recombination lines toward Cassiopeia A: 332 MHz VLA observations and comparison with H I and molecular lines-Reference-Cited by-同舟云学术

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

Published:1994-08 Issue: Volume:430 Page:682
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Anantharamaiah K. R.,Erickson W. C.,Payne H. E.,Kantharia Nimisha G.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 21 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Spectroscopy with the Engineering Development Array: cold H+ at 63 MHz towards the Galactic Centre;Monthly Notices of the Royal Astronomical Society;2019-07-09

2. A high-resolution study of carbon radio recombination lines towards Cassiopeia A;Monthly Notices of the Royal Astronomical Society;2019-03-16

3. Molecular Gas toward Supernova Remnant Cassiopeia A;The Astrophysical Journal;2018-09-17

4. Mapping low-frequency carbon radio recombination lines towards Cassiopeia A at 340, 148, 54, and 43 MHz;Monthly Notices of the Royal Astronomical Society;2017-12-27

5. LOFAR observations of decameter carbon radio recombination lines towards Cassiopeia A;Monthly Notices of the Royal Astronomical Society;2017-01-30

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