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Modeling and predicting the shape of the far-infrared to submillimeter emission in ultra-compact HII regions and cold clumps
D. Paradis, C. Mény, A. Noriega-Crespo +8
Dust properties are very likely affected by the environment in which dust grains evolve. For instance, some analyses of cold clumps (7 K- 17 K) indicate that the aggregation proces…
Dust and Gas in the Magellanic Clouds from the HERITAGE Herschel Key Project. I. Dust Properties and Insights into the Origin of the Submm Excess Emission
Karl D. Gordon, Julia Roman-Duval, Caroline Bot +33
The dust properties in the Large and Small Magellanic Clouds are studied using the HERITAGE Herschel Key Project photometric data in five bands from 100 to 500 micron. Three simple…
The molecular complex associated with the Galactic HII region Sh2-90: a possible site of triggered star formation
M. R. Samal, A. Zavagno, L. Deharveng +6
We investigate the star formation activity in the molecular complex associated with the Galactic HII region Sh2-90, using radio-continuum maps obtained at 1280 MHz and 610 MHz, Her…