2005, IAUS, 227, 346Various physical processes are believed to trigger star formation on the borders of Galactic HII regions. Among these, the collect & collapse process is particularly attractive as it allows the formation of massive objects (single stars or clusters). In order to identify specific cases of this way of triggering star formation we are carrying out a multi-wavelength study of Galactic HII regions that exhibit signposts of massive-star formation at their borders. Hereby, we present two typical examples of such sources and discuss the results in the framework of the collect and collapse process, which seems to be at work as the major triggering agent in these two cases
International audienceThe ``collect and collapse'' model predicts that massive objects−stars or clus...
International audienceThe ``collect and collapse'' model predicts that massive objects−stars or clus...
12 pages, 14 figures. To be published in A&AAims: We wish to establish whether sequential star forma...
2005, IAUS, 227, 346Various physical processes are believed to trigger star formation on the borders...
International audienceYoung massive stars or clusters are often observed at the peripheries of H ii ...
International audienceYoung massive stars or clusters are often observed at the peripheries of H ii ...
International audienceYoung massive stars or clusters are often observed at the peripheries of H ii ...
International audienceYoung massive stars or clusters are often observed at the peripheries of H ii ...
International audienceYoung massive stars or clusters are often observed at the peripheries of H ii ...
International audienceWe discuss a few aspects of star formation triggered by H II regions. We show ...
International audienceWe discuss a few aspects of star formation triggered by H II regions. We show ...
To investigate the process of star formation triggered by the expansion of an HII region, we present...
To investigate the process of star formation triggered by the expansion of an HII region, we present...
International audienceThe ``collect and collapse'' model predicts that massive objects−stars or clus...
International audienceThe ``collect and collapse'' model predicts that massive objects−stars or clus...
International audienceThe ``collect and collapse'' model predicts that massive objects−stars or clus...
International audienceThe ``collect and collapse'' model predicts that massive objects−stars or clus...
12 pages, 14 figures. To be published in A&AAims: We wish to establish whether sequential star forma...
2005, IAUS, 227, 346Various physical processes are believed to trigger star formation on the borders...
International audienceYoung massive stars or clusters are often observed at the peripheries of H ii ...
International audienceYoung massive stars or clusters are often observed at the peripheries of H ii ...
International audienceYoung massive stars or clusters are often observed at the peripheries of H ii ...
International audienceYoung massive stars or clusters are often observed at the peripheries of H ii ...
International audienceYoung massive stars or clusters are often observed at the peripheries of H ii ...
International audienceWe discuss a few aspects of star formation triggered by H II regions. We show ...
International audienceWe discuss a few aspects of star formation triggered by H II regions. We show ...
To investigate the process of star formation triggered by the expansion of an HII region, we present...
To investigate the process of star formation triggered by the expansion of an HII region, we present...
International audienceThe ``collect and collapse'' model predicts that massive objects−stars or clus...
International audienceThe ``collect and collapse'' model predicts that massive objects−stars or clus...
International audienceThe ``collect and collapse'' model predicts that massive objects−stars or clus...
International audienceThe ``collect and collapse'' model predicts that massive objects−stars or clus...
12 pages, 14 figures. To be published in A&AAims: We wish to establish whether sequential star forma...