Carbon and hydrogen radio recombination lines from the cold clouds towards Cassiopeia A
We use the Low Frequency Array to perform a systematic high spectral resolution investigation of the low-frequency 33–78 MHz spectrum along the line of sight to Cassiopeia A. We complement this with a 304–386 MHz Westerbork Synthesis Radio Telescope observation. In this first paper, we focus on the...
Váldodahkkit: | Oonk, J, van Weeren, R, Salas, P, Salgado, F, Morabito, L, Toribio, M, Tielens, A, Röttgering, H |
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Materiálatiipa: | Journal article |
Almmustuhtton: |
Oxford University Press
2017
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Geahča maid
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LOFAR observations of decameter carbon radio recombination lines towards Cassiopeia A
Dahkki: Salas, P, et al.
Almmustuhtton: (2017) -
Low-frequency carbon radio recombination lines. I. Calculations of departure coefficients
Dahkki: Salgado, F, et al.
Almmustuhtton: (2017) -
Low-frequency carbon radio recombination lines. II. The diffuse interstellar medium
Dahkki: Salgado, F, et al.
Almmustuhtton: (2017) -
LOFAR detections of low-frequency radio recombination lines towards
Cassiopeia A
Dahkki: Asgekar, A, et al.
Almmustuhtton: (2013) -
Discovery of carbon radio recombination lines in absorption towards Cygnus A
Dahkki: Oonk, J, et al.
Almmustuhtton: (2014)