Volume 563, March 2014
|Number of page(s)||22|
|Section||Interstellar and circumstellar matter|
|Published online||03 March 2014|
Gaussian fitting results.
H66α radio recombination line spectra. “Gaussian 1”, the component with the higher velocity, is shown in red, and “Gaussian 2” in blue (Table 2). The dashed black line presents the sum of the two Gaussian fits. The vertical black line marks the systemic molecular gas velocity of − 1.5 km s-1.
|Open with DEXTER|
© ESO, 2014
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