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A massive prestellar clump hosting no high-mass cores
(IOP Publishing, 2017-06-01)
The infrared dark cloud (IRDC) G028.23-00.19 hosts a massive (1500M(circle dot)), cold (12 K), and 3.6-70 mu m IR dark clump (MM1) that has the potential to form high-mass stars. We observed this prestellar clump candidate ...
A molecular outflow revealing star formation activity in the vicinity of the HII region G034.8-0.7 and the SNR W44
(EDP Sciences, 2009-05)
Aims. This work aims at investigating the molecular gas component in the vicinity of two young stellar object (YSO) candidates identified at the border of the HII region G034.8-0.7 that is evolving within a molecular cloud ...
The low-frequency radio emission and spectrum of the extended SNR W44: new VLA observations at 74 and 324 MHz
(EDP Sciences, 2007-12)
Aims. We present new Very Large Array (VLA) radio images at 74 and 324 MHz of the SNR W44. The VLA images, obtained with unprecedented angular resolution and sensitivity for such low frequencies (HPBW 37 at 74 MHz, and 13 ...
New VLA observations of the SNR Puppis A : the radio properties and the correlation with the X-ray emission
(EDP Sciences, 2006-12)
Context. High-resolution, high-sensitivity multifrequency radio images of supernova remnants (SNRs) are essential in advancing the understanding of both the global SNR dynamics and particle acceleration mechanisms. Aims. ...
Molecular Line Emission Towards High-Mass Clumps: The MALT90 Catalogue
(Cambridge University Press, 2016)
The Millimetre Astronomy Legacy Team 90 GHz survey aims to characterise the physical and chemical evolution of high-mass clumps. Recently completed, it mapped 90 GHz line emission towards 3 246 high-mass clumps identified ...