Abstract
We mapped 4 bright-rimmed clouds in IC 1396 in the veloci-ty–resolved [C ii] 158 μm emission, and analyzed the dynamics of gas components traced by [C ii] and CO. In all rims the [C ii] emission is not fully reproduced by the CO line profile, indicating a complex origin of the line emission including ablating material.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Paper version not known
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
