We present 1.2-arcmin resolution images of the Galactic H II regions W43 and M17 made with the Very Large Array (VLA) at a frequency of 330 MHz; these are the highest resolution images to date of the large-scale structures of these complexes at any frequency. The electron temperature towards the component of W43 that has the highest emission measure, G30.8-0.0, is 5410 ± 300 K. The electron temperatures towards the components of M17, G15.0 - 0.7 and G15.1 - 0.7, are 7600−210+700 and 8000−220+450 K respectively. These estimates are consistent with previous estimates based on radio recombination line and continuum observations of these H II regions
We report multifrequency radio continuum and hydrogen radio recombination line observations of HII r...
We present a 1.1-arcmin-resolution image of the W51 complex made with the Very Large Array at a freq...
Far-infrared and radio continuum maps have been made of the central 6' of the inner-galaxy H II regi...
We present radio continuum images of three Galactic H Ii regions, S 201, S 206, and S 209 near 232, ...
We present radio continuum images of three Galactic H II regions, S 201, S 206, and S 209 near 232, ...
We present high-sensitivity, high-resolution VLA observations of the W3 complex of H II regions in t...
Spectral data are presented, giving intensities of the Brackett ɤ (B7) line at six positions in M 42...
Presented at the 21st meeting of the Astronomical Society of India, Pune, 2002.Three Galactic HII re...
We have compiled a catalogue of H ii regions detected with the Murchison Widefield Array between 72 ...
We have imaged the large-scale radio continuum structure in the Orion region with the Very Large Arr...
We have compiled a catalogue of H II regions detected with the Murchison Widefield Array between 72 ...
© Astronomical Society of Australia 2016. We have compiled a catalogue of H ii regions detected with...
We have carried out VLA radio continuum (6 and 20cm), VLA HI 21cm line, and 13CO J = 1 --\u3e 0 line...
Based on the idea that star formation goes on progressively in molecular clouds, a search was conduc...
We present high-sensitivity, high-resolution VLA observations of the W3 complex of H II regions in t...
We report multifrequency radio continuum and hydrogen radio recombination line observations of HII r...
We present a 1.1-arcmin-resolution image of the W51 complex made with the Very Large Array at a freq...
Far-infrared and radio continuum maps have been made of the central 6' of the inner-galaxy H II regi...
We present radio continuum images of three Galactic H Ii regions, S 201, S 206, and S 209 near 232, ...
We present radio continuum images of three Galactic H II regions, S 201, S 206, and S 209 near 232, ...
We present high-sensitivity, high-resolution VLA observations of the W3 complex of H II regions in t...
Spectral data are presented, giving intensities of the Brackett ɤ (B7) line at six positions in M 42...
Presented at the 21st meeting of the Astronomical Society of India, Pune, 2002.Three Galactic HII re...
We have compiled a catalogue of H ii regions detected with the Murchison Widefield Array between 72 ...
We have imaged the large-scale radio continuum structure in the Orion region with the Very Large Arr...
We have compiled a catalogue of H II regions detected with the Murchison Widefield Array between 72 ...
© Astronomical Society of Australia 2016. We have compiled a catalogue of H ii regions detected with...
We have carried out VLA radio continuum (6 and 20cm), VLA HI 21cm line, and 13CO J = 1 --\u3e 0 line...
Based on the idea that star formation goes on progressively in molecular clouds, a search was conduc...
We present high-sensitivity, high-resolution VLA observations of the W3 complex of H II regions in t...
We report multifrequency radio continuum and hydrogen radio recombination line observations of HII r...
We present a 1.1-arcmin-resolution image of the W51 complex made with the Very Large Array at a freq...
Far-infrared and radio continuum maps have been made of the central 6' of the inner-galaxy H II regi...