Add to ORKGThe property of dust in four southern H II region/molecular cloud complexes (RCW 108, RCW 57, RCW 122, and G351.6-1.3) was discussed. These regions were observed at an effective wavelength of 150 micron using TIFR balloon borne 1 m telescope and deconvolved maps with a resolution of 1 min were obtained. The data were combined with other available data to derive the properties of the infrared emitting dust in these regions
Several 1.0 continuum mapping observations were made of seven southern hemisphere h12/molecular clou...
International audienceContext. RCW 120 is a well-studied, nearby Galactic HII region with ongoing st...
International audienceWe study infrared emission of 17 isolated, diffuse clouds with masses of order...
W31 is a H II region/molecular cloud complex in the galactic plane at a distance of 6 Kpc. This comp...
The analysis of several diffuse interstellar clouds observed by the Infrared Astronomy Satellite (IR...
The distributions of physical properties, such as the temperature, mass, or density of the dust grai...
We have analyzed IRAS maps at 60 and 100-mu-m of the complex of dark clouds containing L134, L183 an...
Context. LDN 1642 is a rare example of a star-forming, high-latitude molecular cloud. The dust emiss...
We present a study of the dust properties of 12 classical and superbubble H II regions in the Large ...
Context. Lynds 1780 is a high-latitude cloud where, based on 2MASS, the maximum visual extinction is...
A catalog of southern dust cloud properties is being compiled to aid in the planning and analysis of...
Because infrared emission is a very good tracer of mass at high latitudes, by combining it with HI o...
Observations of three southern H II regions, namely RCW 57, RCW 108, and RCW 122, in a 120-300 micro...
As a model for infrared sources in molecular regions, we calculate the radiative transfer in a dust ...
Context. Because of their relatively simple morphology, “bubble” H II regions have been instrumental...
Several 1.0 continuum mapping observations were made of seven southern hemisphere h12/molecular clou...
International audienceContext. RCW 120 is a well-studied, nearby Galactic HII region with ongoing st...
International audienceWe study infrared emission of 17 isolated, diffuse clouds with masses of order...
W31 is a H II region/molecular cloud complex in the galactic plane at a distance of 6 Kpc. This comp...
The analysis of several diffuse interstellar clouds observed by the Infrared Astronomy Satellite (IR...
The distributions of physical properties, such as the temperature, mass, or density of the dust grai...
We have analyzed IRAS maps at 60 and 100-mu-m of the complex of dark clouds containing L134, L183 an...
Context. LDN 1642 is a rare example of a star-forming, high-latitude molecular cloud. The dust emiss...
We present a study of the dust properties of 12 classical and superbubble H II regions in the Large ...
Context. Lynds 1780 is a high-latitude cloud where, based on 2MASS, the maximum visual extinction is...
A catalog of southern dust cloud properties is being compiled to aid in the planning and analysis of...
Because infrared emission is a very good tracer of mass at high latitudes, by combining it with HI o...
Observations of three southern H II regions, namely RCW 57, RCW 108, and RCW 122, in a 120-300 micro...
As a model for infrared sources in molecular regions, we calculate the radiative transfer in a dust ...
Context. Because of their relatively simple morphology, “bubble” H II regions have been instrumental...
Several 1.0 continuum mapping observations were made of seven southern hemisphere h12/molecular clou...
International audienceContext. RCW 120 is a well-studied, nearby Galactic HII region with ongoing st...
International audienceWe study infrared emission of 17 isolated, diffuse clouds with masses of order...