We characterize an uncatalogued bright-rimmed cloud located onto the border of the infrared dust bubble CN20 in order to investigate triggered star formation. To do this, we carried out radio continuum observations at 8.9 GHz with the Jansky Very Large Array (JVLA) interferometer with a synthesized beam of 13′′× 5′′, and molecular observations using the Atacama Submillimeter Telescope Experiment (ASTE) in the 12CO J=3?2 and CS J=7?6 transitions. The analysis of the molecular observations and Herschel public data reveals the presence of a warm and dense clump with Tdust 25 K and n(H2) 3 × 105 cm−3. The high angular resolution and sensitivity of the new radio continuum data have revealed an arc-like radio filament in excellent correspondence...
We studied the environment of the dust bubble N10 in molecular emission. Infrared bubbles, first det...
We present a multi-wavelength investigation of the H ii region G347.600+00.211, located at a distanc...
We investigate the presence of molecular gas associated with the infrared dust bubble S,24 based on...
We characterize an uncatalogued bright-rimmed cloud located at the border of the infrared dust bubbl...
Artículo de publicación ISI.Aims. We characterize a bright-rimmed cloud embedded in the H II region ...
Aims. To characterize a bright-rimmed cloud embedded in the Hii region Sh2-48 searching for evidence...
Using molecular lines and radio continuum observations, Ortega et al. (2016) studied the bright-rimm...
We have carried out an archival radio, optical and infrared wavelength imaging survey of 44 Bright-R...
Context. Bright-rimmed clouds (BRCs) are isolated molecular clouds located on the edges of evolved H...
Aims. To search for evidence of triggered star formation within four bright-rimmed clouds, SFO 58, S...
We present the results of an in-depth study of four bright-rimmed clouds (BRCs), SFO 58, SFO 68, SFO...
We have carried out an archival radio, optical and infrared wavelength imaging survey of 44 Bright-R...
We have carried out a radio-wavelength imaging survey of 45 bright-rimmed clouds (BRCs), using the A...
We have carried out a radio-wavelength imaging survey of 45 bright-rimmed clouds (BRCs), using the A...
A sample of optically Bright-Rimmed Clouds (BRC) at the edge of HII regions has been observed at mul...
We studied the environment of the dust bubble N10 in molecular emission. Infrared bubbles, first det...
We present a multi-wavelength investigation of the H ii region G347.600+00.211, located at a distanc...
We investigate the presence of molecular gas associated with the infrared dust bubble S,24 based on...
We characterize an uncatalogued bright-rimmed cloud located at the border of the infrared dust bubbl...
Artículo de publicación ISI.Aims. We characterize a bright-rimmed cloud embedded in the H II region ...
Aims. To characterize a bright-rimmed cloud embedded in the Hii region Sh2-48 searching for evidence...
Using molecular lines and radio continuum observations, Ortega et al. (2016) studied the bright-rimm...
We have carried out an archival radio, optical and infrared wavelength imaging survey of 44 Bright-R...
Context. Bright-rimmed clouds (BRCs) are isolated molecular clouds located on the edges of evolved H...
Aims. To search for evidence of triggered star formation within four bright-rimmed clouds, SFO 58, S...
We present the results of an in-depth study of four bright-rimmed clouds (BRCs), SFO 58, SFO 68, SFO...
We have carried out an archival radio, optical and infrared wavelength imaging survey of 44 Bright-R...
We have carried out a radio-wavelength imaging survey of 45 bright-rimmed clouds (BRCs), using the A...
We have carried out a radio-wavelength imaging survey of 45 bright-rimmed clouds (BRCs), using the A...
A sample of optically Bright-Rimmed Clouds (BRC) at the edge of HII regions has been observed at mul...
We studied the environment of the dust bubble N10 in molecular emission. Infrared bubbles, first det...
We present a multi-wavelength investigation of the H ii region G347.600+00.211, located at a distanc...
We investigate the presence of molecular gas associated with the infrared dust bubble S,24 based on...