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A protostellar jet emanating from a hypercompact H II region
(The American Astronomical Society, 2016)
We present radio continuum observations of the high-mass young stellar object (HMYSO) G345.4938+01.4677
obtained using the Australia Telescope Compact Array (ATCA) at 5, 9, 17, and 19 GHz. These observations
provide ...
A Protostellar Jet Emanating from a hypercompact H II Region
(IOP, 2016)
We present radio continuum observations of the high-mass young stellar object (HMYSO) G345.4938+01.4677 obtained using the Australia Telescope Compact Array (ATCA) at 5, 9, 17, and 19 GHz. These observations provide definite ...
Análisis de la región de formación estelar vinculada a la fuente IRAS 15492-5426
(Asociación Argentina de Astronomía, 2021-07)
A study was conducted on the star formation region linked to the IRAS source 15492-546 located in the complex G327.3-0.5. This one consists of a dark molecular cloud in which the emission of their molecules has been studied ...
Multiwavelength studies of WR 21a and its surroundings
(EDP Sciences, 2005-12)
We present results of high-resolution radio continuum observations towards the binary star WR 21a (Wack 2134) obtained with the Australia Telescope Compact Array (ATCA ) at 4.8 and 8.64 GHz. We detected the system at 4.8 ...
The molecular environment of the Galactic star forming region G19.61–0.23
(ESO, 2010-06-03)
Context. Although current facilities allow the study of Galactic star formation at high angular resolution, our current understanding
of the high-mass star-formation process is still very poor. In particular, we still ...
The molecular complex associated with RCW121 and RCW122
(EDP Sciences, 2008-05)
Aims. We analyse the distribution of the molecular gas towards the region containing the open cluster Havlen-Moffat 1 (HM 1) the Wolf-Rayet stars WR 87, WR 89, and WR 91, and the star forming regions RCW 121 and RCW 122, ...
Candidate counterparts to the soft gamma-ray flare in the direction of LS I +61 303
(EDP Sciences, 2009-04)
Context: A short duration burst reminiscent of a soft gamma-ray repeater/anomalous X-ray pulsar behaviour was detected in the direction of LS I +61 303 by the Swift satellite. While the association with this well known ...