Volume 560, December 2013
|Number of page(s)||5|
|Published online||05 December 2013|
Profiles of the N-rich species CN and NS observed for IRC +10420. The hyperfine components of these transitions cannot be resolved due to the high expansion velocity of this object. The different hyperfine transitions of each species are represented by the ticks in the line below the profile.
|Open with DEXTER|
© ESO, 2013
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