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...
Главные авторы: | Oonk, J, van Weeren, R, Salas, P, Salgado, F, Morabito, L, Toribio, M, Tielens, A, Röttgering, H |
---|---|
Формат: | Journal article |
Опубликовано: |
Oxford University Press
2017
|
Схожие документы
-
LOFAR observations of decameter carbon radio recombination lines towards Cassiopeia A
по: Salas, P, и др.
Опубликовано: (2017) -
Low-frequency carbon radio recombination lines. I. Calculations of departure coefficients
по: Salgado, F, и др.
Опубликовано: (2017) -
Low-frequency carbon radio recombination lines. II. The diffuse interstellar medium
по: Salgado, F, и др.
Опубликовано: (2017) -
LOFAR detections of low-frequency radio recombination lines towards
Cassiopeia A
по: Asgekar, A, и др.
Опубликовано: (2013) -
Discovery of carbon radio recombination lines in absorption towards Cygnus A
по: Oonk, J, и др.
Опубликовано: (2014)