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AIMS: We investigate the environment of the infrared dust bubble N65 andsearch for evidence of triggered star formation in its surroundings. METHODS:We performed a multiwavelength study of the region around N65 with data takenfrom large-scale surveys: Two Micron All Sky Survey, GLIMPSE, MIPSGAL, SCUBA,and GRS. We analyzed the distribution of the molecular gas and dust in theenvironment of N65 and performed infrared photometry and spectral analysis ofpoint sources to search for young stellar objects and identify the ionizingstar candidates. RESULTS: We found a molecular cloud that appears to befragmented into smaller clumps along the N65 PDR. This indicates that theso-called collect and collapse process may be occurring. Several young stellarobjects are distributed among the molecular clumps. They may represent a secondgeneration of stars whose formation was triggered by the bubble expanding intothe molecular gas. We dentified O-type stars inside N65, which are the mostreliable ionizing star candidates.

The environment of the infrared dust bubble N65: a mutiwavelength study