Context. IC 1396N is a bright-rimmed cloud associated with an intermediate-mass star-forming region, where a number of Herbig-Haro objects, H2 jet-like features, CO molecular outflows, and millimeter compact sources have been observed. Aims. We study the complex structure of the IC 1396N core and the molecular outflows detected in the region in detail and reveal the presence of additional YSOs inside this globule. Methods. We carried out a deep survey of the IC 1396N region in the $J, H, K'$ broadband filters and deep high-angular resolution observations in the H2 narrowband filter with NICS at the TNG telescope. The completeness limits in the 2MASS standard are $K_{\rm s} \sim 17.5$, $H \sim 18.5$, and $J \sim 19.5$. ...
Context. The IC 1396 A globule, located to the west of the young cluster Tr 37, is known to host man...
We have carried out an in-depth study of three bright-rimmed clouds SFO 11, SFO 11NE and SFO 11E ass...
Rich young stellar clusters produce H?ii regions whose expansion into the nearby molecular cloud is ...
Context. IC 1396N is a bright-rimmed cloud associated with an intermediate-mass star-forming region,...
We have observed the IC 1396 W globule in a narrow band filter centred on the 1-0 S(1) line of molec...
International audienceWe present a large-scale study of the IC 1396 region using new deep NIR and op...
Context. The IC 1396 A globule, located to the west of the young cluster Tr 37, is known to host man...
Context. The IC 1396 A globule, located to the west of the young cluster Tr 37, is known to host man...
Context. The bright-rimmed cloud IC 1396N, associated with an intermediate-mass star-forming region,...
Artículo de publicación ISI.Aims. We characterize a bright-rimmed cloud embedded in the H II region ...
Context. The IC 1396 A globule, located to the west of the young cluster Tr 37, is known t...
We have observed the IC1396W globule in a narrow band filter centred on the 1-0 S(1) line of molecul...
Context. The IC 1396 A globule, located to the west of the young cluster Tr 37, is known to host man...
Aims. To advance our knowledge of star formation, in addition to statistical studies and large surve...
International audienceContext: .Massive-star formation triggered by the expansion of H ii regions. A...
Context. The IC 1396 A globule, located to the west of the young cluster Tr 37, is known to host man...
We have carried out an in-depth study of three bright-rimmed clouds SFO 11, SFO 11NE and SFO 11E ass...
Rich young stellar clusters produce H?ii regions whose expansion into the nearby molecular cloud is ...
Context. IC 1396N is a bright-rimmed cloud associated with an intermediate-mass star-forming region,...
We have observed the IC 1396 W globule in a narrow band filter centred on the 1-0 S(1) line of molec...
International audienceWe present a large-scale study of the IC 1396 region using new deep NIR and op...
Context. The IC 1396 A globule, located to the west of the young cluster Tr 37, is known to host man...
Context. The IC 1396 A globule, located to the west of the young cluster Tr 37, is known to host man...
Context. The bright-rimmed cloud IC 1396N, associated with an intermediate-mass star-forming region,...
Artículo de publicación ISI.Aims. We characterize a bright-rimmed cloud embedded in the H II region ...
Context. The IC 1396 A globule, located to the west of the young cluster Tr 37, is known t...
We have observed the IC1396W globule in a narrow band filter centred on the 1-0 S(1) line of molecul...
Context. The IC 1396 A globule, located to the west of the young cluster Tr 37, is known to host man...
Aims. To advance our knowledge of star formation, in addition to statistical studies and large surve...
International audienceContext: .Massive-star formation triggered by the expansion of H ii regions. A...
Context. The IC 1396 A globule, located to the west of the young cluster Tr 37, is known to host man...
We have carried out an in-depth study of three bright-rimmed clouds SFO 11, SFO 11NE and SFO 11E ass...
Rich young stellar clusters produce H?ii regions whose expansion into the nearby molecular cloud is ...