Aims. We present a multiwavelength analysis of the infrared dust bubble S 24 and the extended IR sources G341.220-0.213 and G341.217-0.237 located in its environs. We aim to investigate the characteristics of the molecular gas and the interstellar dust linked to them and analyze the evolutionary state of the young stellar objects identified there and the relation of the bubble to S 24 and the IR sources. Methods. Using the APEX telescope, we mapped the molecular emission in the CO(2-1), 13CO(2-1), C18O(2-1), and 13CO(3-2) lines in a region of about 5′ × 5′ in size around the bubble. The cold dust distribution was analyzed using submillimeter continuum images from ATLASGAL and Herschel. Complementary IR and radio data at different wavelength...
Aims. With the aim of investigating the presence of molecular and dust clumps linked to two star for...
Aims. We analyze the distribution of the molecular gas and dust in the molecular clump linked to IRA...
Aims. This work aims at investigating the molecular and infrared components in the massive young st...
Aims. We present a multiwavelength analysis of the infrared dust bubble S 24 and the extended IR sou...
Aims. We present a multi-wavelength analysis of the infrared dust bubble S 24, and the extended IR s...
Aims. We present a multiwavelength analysis of the infrared dust bubble S 24 and the extended IR sou...
Aims. We present a multiwavelength analysis of the infrared dust bubble S 24 and the extended IR sou...
Basados en la emisión molecular en las líneas 12CO(2-1) y 13CO(2-1), y en la emisión en el continuo ...
We investigate the presence of molecular gas associated with the infrared dust bubble S,24 based on...
We present an analysis of YSOs linked to the IR dust bubble complex S21-S22-S23-S24 of about 12 arcm...
Based on the molecular emission in the 12CO(2-1) and 13CO(2-1) lines, and on the continuum emission ...
The MIPSGAL 24 μm Galactic Plane Survey has revealed more than 400 compact-extended objects. Less th...
The MIPSGAL 24 μm Galactic Plane Survey has revealed more than 400 compact-extended objects. Less t...
We present a multi-wavelength study of the IR bubble G24.136+00.436. The J = 1-0 observations of (CO...
Aims. This work aims at investigating the molecular gas component in the vicinity of two young stell...
Aims. With the aim of investigating the presence of molecular and dust clumps linked to two star for...
Aims. We analyze the distribution of the molecular gas and dust in the molecular clump linked to IRA...
Aims. This work aims at investigating the molecular and infrared components in the massive young st...
Aims. We present a multiwavelength analysis of the infrared dust bubble S 24 and the extended IR sou...
Aims. We present a multi-wavelength analysis of the infrared dust bubble S 24, and the extended IR s...
Aims. We present a multiwavelength analysis of the infrared dust bubble S 24 and the extended IR sou...
Aims. We present a multiwavelength analysis of the infrared dust bubble S 24 and the extended IR sou...
Basados en la emisión molecular en las líneas 12CO(2-1) y 13CO(2-1), y en la emisión en el continuo ...
We investigate the presence of molecular gas associated with the infrared dust bubble S,24 based on...
We present an analysis of YSOs linked to the IR dust bubble complex S21-S22-S23-S24 of about 12 arcm...
Based on the molecular emission in the 12CO(2-1) and 13CO(2-1) lines, and on the continuum emission ...
The MIPSGAL 24 μm Galactic Plane Survey has revealed more than 400 compact-extended objects. Less th...
The MIPSGAL 24 μm Galactic Plane Survey has revealed more than 400 compact-extended objects. Less t...
We present a multi-wavelength study of the IR bubble G24.136+00.436. The J = 1-0 observations of (CO...
Aims. This work aims at investigating the molecular gas component in the vicinity of two young stell...
Aims. With the aim of investigating the presence of molecular and dust clumps linked to two star for...
Aims. We analyze the distribution of the molecular gas and dust in the molecular clump linked to IRA...
Aims. This work aims at investigating the molecular and infrared components in the massive young st...