DOIAbstract
Aims. We report the first spectroscopic mapping of an atomic carbon line in an infrared dark cloud (IRDC). By observing the spatial distribution of the [C
Aims. We report the first spectroscopic mapping of an atomic carbon line in an infrared dark cloud (IRDC). By observing the spatial distribution of the [C
High-resolution spectra of the 158 μm fine-structure line of ionized carbon have been obtained with ...
We present spectral data cubes of the [CI] 809 GHz, 12CO 115 GHz, 13CO 110 GHz, and HI 1.4 GHz line ...
Large-scale mapping observations of the 3P1–3P0 fine-structure transition of atomic carbon (C i, 492...
Aims. We report the first spectroscopic mapping of an atomic carbon line in an infrared da...
<BR /> Aims: We report the first spectroscopic mapping of an atomic carbon line in an infrared dark ...
Infrared dark clouds (IRDCs) are potential sites of massive star formation, dark in the near-infrare...
Context. How molecular clouds form out of the atomic phase and what the relative fractions of carbon...
Context. How molecular clouds form out of the atomic phase and what the relative fractions of carbon...
We present observations of the 3P1-3P0 fine-structure transition of atomic carbon [CI], the J=3-2 tr...
Although carbon is the fourth most cosmically abundant element, it exists only rarely as neutral ato...
Context. IRC +10216 is the prototypical carbon star exhibiting an extended molecular circu...
We have mapped the C I 3P1-3P0 line at 492 GHzin three molecular clouds immersed in weak ultraviolet...
Context. IRC +10216 is the prototypical carbon star exhibiting an extended molecular circumstellar e...
High-resolution spectra of the 158 μm fine-structure line of ionized carbon have been obtained with ...
We present spectral data cubes of the [CI] 809 GHz, 12CO 115 GHz, 13CO 110 GHz, and HI 1.4 GHz line ...
Large-scale mapping observations of the 3P1–3P0 fine-structure transition of atomic carbon (C i, 492...
Aims. We report the first spectroscopic mapping of an atomic carbon line in an infrared da...
<BR /> Aims: We report the first spectroscopic mapping of an atomic carbon line in an infrared dark ...
Infrared dark clouds (IRDCs) are potential sites of massive star formation, dark in the near-infrare...
Context. How molecular clouds form out of the atomic phase and what the relative fractions of carbon...
Context. How molecular clouds form out of the atomic phase and what the relative fractions of carbon...
We present observations of the 3P1-3P0 fine-structure transition of atomic carbon [CI], the J=3-2 tr...
Although carbon is the fourth most cosmically abundant element, it exists only rarely as neutral ato...
Context. IRC +10216 is the prototypical carbon star exhibiting an extended molecular circu...
We have mapped the C I 3P1-3P0 line at 492 GHzin three molecular clouds immersed in weak ultraviolet...
Context. IRC +10216 is the prototypical carbon star exhibiting an extended molecular circumstellar e...
High-resolution spectra of the 158 μm fine-structure line of ionized carbon have been obtained with ...
We present spectral data cubes of the [CI] 809 GHz, 12CO 115 GHz, 13CO 110 GHz, and HI 1.4 GHz line ...
Large-scale mapping observations of the 3P1–3P0 fine-structure transition of atomic carbon (C i, 492...
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