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We present a study on the molecular gas towards a bright-rimmed cloud locatedto the north of the infrared dust bubble N30. Using the emission from the 12CO,13CO, and C18O J=3-2 line, together with infrared and radio continuum data, wecharacterized the bubble and the related molecular cloud. In addition, we showan analysis of the behaviour of the abundance ratio 13CO/C18O towards thebright-rimmed cloud, and we search for clues on recent star-formation.

Studying the molecular gas towards a bright rimmed cloud at the infrared dust bubble N30