Add to ORKGMassive stars are known to play an important role in energizing the interstellar medium; however, their formation mechanism is still not well understood. In this study, we have identified compact HII regions around massive young stellar object so that follow-up observations can be made to study how massive stars are formed and how they affect the dynamics of the ambient cloud material in their early lifetime.Ope
International audienceThe aim of this study is to characterize the distribution and basic properties...
We have compiled the most complete compact and ultracompact HII region catalogue to date via multi-w...
Aims: As a continuation of a previous work, in which we found strong evidence of massive molecular ...
Massive stars are known to play an important role in energizing the interstellar medium; however, th...
This thesis presents an analysis of the largest catalog to date of infrared spectra of massive young...
The H II complex N 159 in the Large Magellanic Cloud is used to study massive star formation in diff...
International audienceThe H II complex N 159 in the Large Magellanic Cloud is used to study massive ...
We present and categorize Spitzer infrared spectrometer spectra of 294 objects in the Large Magellan...
Massive stars form in the dense optically thick cores of molecular clouds throughout the Galaxy. The...
11 pages, 10 figures. To be published in A&AContext. Massive-star formation triggered by the expansi...
International audienceWe present our results on high resolution imaging and spectroscopy using the H...
Context. High-mass stars form in much richer environments than those associated with isolated low-ma...
12 pages, 14 figures. To be published in A&AAims: We wish to establish whether sequential star forma...
International audienceContext. The region of the Small Magellanic Cloud (SMC) with which this paper ...
Context. Young massive stars and stellar clusters continuously form in the Galactic disk, generating...
International audienceThe aim of this study is to characterize the distribution and basic properties...
We have compiled the most complete compact and ultracompact HII region catalogue to date via multi-w...
Aims: As a continuation of a previous work, in which we found strong evidence of massive molecular ...
Massive stars are known to play an important role in energizing the interstellar medium; however, th...
This thesis presents an analysis of the largest catalog to date of infrared spectra of massive young...
The H II complex N 159 in the Large Magellanic Cloud is used to study massive star formation in diff...
International audienceThe H II complex N 159 in the Large Magellanic Cloud is used to study massive ...
We present and categorize Spitzer infrared spectrometer spectra of 294 objects in the Large Magellan...
Massive stars form in the dense optically thick cores of molecular clouds throughout the Galaxy. The...
11 pages, 10 figures. To be published in A&AContext. Massive-star formation triggered by the expansi...
International audienceWe present our results on high resolution imaging and spectroscopy using the H...
Context. High-mass stars form in much richer environments than those associated with isolated low-ma...
12 pages, 14 figures. To be published in A&AAims: We wish to establish whether sequential star forma...
International audienceContext. The region of the Small Magellanic Cloud (SMC) with which this paper ...
Context. Young massive stars and stellar clusters continuously form in the Galactic disk, generating...
International audienceThe aim of this study is to characterize the distribution and basic properties...
We have compiled the most complete compact and ultracompact HII region catalogue to date via multi-w...
Aims: As a continuation of a previous work, in which we found strong evidence of massive molecular ...