The infrared dust bubble N22: an expanding H II region and the star formation around it

Aims. To increase the observational samples of star formation around expanding H II regions, we analyzed the interstellar medium and star formation around N22. Methods. We used data extracted from the seven large-scale surveys from infrared to radio wavelengths. In addition we used the JCMT(star) observations of the J = 3-2 line of (CO)-C-12 emission data released on CADC(star star) and the (CO)-C-12 J = 2-1 and J = 3-2 lines observed by the KOSMA(star star star) 3 m telescope. We performed a multiwavelength study of bubble N22. Results. A molecular shell composed of several clumps agrees very well with the border of N22, suggesting that its expansion is collecting the surrounding material. The high integrated (CO)-C-12 line intensity ratio RICO(3-2)/ICO(2-1) (ranging from 0.7 to 1.14) implies that shocks have driven into the molecular clouds. We identify eleven possible O-type stars inside the H II region, five of which are located in projection inside the cavity of the 20 cm radio continuum emission and are probably the exciting-star candidates of N22. Twenty-nine young stellar objects (YSOs) are distributed close to the dense cores of N22. We conclude that star formation is indeed active around N22; the formation of most of YSOs may have been triggered by the expanding of the H II region. After comparing the dynamical age of N22 and the fragmentation time of the molecular shell, we suggest that radiation-driven compression of pre-existing dense clumps may be ongoing.Astronomy & AstrophysicsSCI(E)EI7ARTICLEnull54