Context. The presence and properties of compact radio sources embedded in massive star forming regions can reveal important physical properties about these regions and the processes occurring within them. The NGC 6334 complex, a massive star forming region, has been studied extensively. Nevertheless, none of these studies has focused in its content in compact radio sources. Aims. Our goal here is to report on a systematic census of the compact radio sources toward NGC 6334, and their characteristics. This will be used to attempt to define their very nature. Methods. We used the VLA C band (4–8 GHz) archive data with 0.̋36 (500 AU) of spatial resolution and noise level of 50 μJy bm−1 to carry out a systematic search for compact radio sources...
We present new multi-frequency radio continuum imaging of the dwarf starburst galaxy NGC 625 obtaine...
This paper presents a study of the rate and efficiency of star formation in the NGC 6334 star formin...
International audienceAims. The formation of high-mass stars is still debated. For this reason, seve...
Context. The presence and properties of compact radio sources embedded in massive star forming regio...
We present results of high-sensitivity, high-resolution, multifrequency VLA observations toward the ...
[[abstract]]We present sensitive, high angular resolution 1.3 cm and 7 mm observations of the massiv...
Infrared photometry and maps from 2 to 100 microns are presented for three of the principal far infr...
NGC 6334 is a galactic star-forming region in Scorpius, heavily obscured by intervening dust. The re...
Aims. We aim to characterise certain physical properties of high-mass star-forming sites in the NGC ...
NGC 6334 (1=351°.1, b=0°.7, distance = 1.7 kpc) is a region where multiple star formation has occurr...
International audienceWe have observed NGC 6334 with NASA's Spitzer Space Telescope, using the IRAC ...
The noise level in the central part of the field is 11 Jy. From these data we have extracted a catal...
We present new multifrequency radio continuum imaging of the dwarf starburst galaxy NGC 625 obtained...
Aims. The formation of high-mass stars is still debated. For this reason, several projects such as H...
We present sensitive, high angular resolution 1.3 cm and 7 mm observations of the massive core NGC 6...
We present new multi-frequency radio continuum imaging of the dwarf starburst galaxy NGC 625 obtaine...
This paper presents a study of the rate and efficiency of star formation in the NGC 6334 star formin...
International audienceAims. The formation of high-mass stars is still debated. For this reason, seve...
Context. The presence and properties of compact radio sources embedded in massive star forming regio...
We present results of high-sensitivity, high-resolution, multifrequency VLA observations toward the ...
[[abstract]]We present sensitive, high angular resolution 1.3 cm and 7 mm observations of the massiv...
Infrared photometry and maps from 2 to 100 microns are presented for three of the principal far infr...
NGC 6334 is a galactic star-forming region in Scorpius, heavily obscured by intervening dust. The re...
Aims. We aim to characterise certain physical properties of high-mass star-forming sites in the NGC ...
NGC 6334 (1=351°.1, b=0°.7, distance = 1.7 kpc) is a region where multiple star formation has occurr...
International audienceWe have observed NGC 6334 with NASA's Spitzer Space Telescope, using the IRAC ...
The noise level in the central part of the field is 11 Jy. From these data we have extracted a catal...
We present new multifrequency radio continuum imaging of the dwarf starburst galaxy NGC 625 obtained...
Aims. The formation of high-mass stars is still debated. For this reason, several projects such as H...
We present sensitive, high angular resolution 1.3 cm and 7 mm observations of the massive core NGC 6...
We present new multi-frequency radio continuum imaging of the dwarf starburst galaxy NGC 625 obtaine...
This paper presents a study of the rate and efficiency of star formation in the NGC 6334 star formin...
International audienceAims. The formation of high-mass stars is still debated. For this reason, seve...