The Millimetre Astronomy Legacy Team 90 GHz (MALT90) survey aims to characterise the physical and chemical evolution of high-mass star-forming clumps. Exploiting the unique broad frequency range and on-the-fly mapping capabilities of the Australia Telescope National Facility Mopra 22 m single-dish telescope 1 , MALT90 has obtained 3? × 3? maps towards ~2 000 dense molecular clumps identified in the ATLASGAL 870 ?m Galactic plane survey. The clumps were selected to host the early stages of high-mass star formation and to span the complete range in their evolutionary states (from prestellar, to protostellar, and on to H II regions and photodissociation regions). Because MALT90 mapped 16 lines simultaneously with excellent spatial (38 arcsec) ...
I studied the formation of massive stars and clusters via millimeter, radio, and infrared observatio...
We characterise the Millimetre Astronomy Legacy Team 90 GHz Survey (MALT90) and the Mopra telescope ...
We report Atacama Large Millimeter Array observations of 3 mm dust continuum emission and line emiss...
The Millimetre Astronomy Legacy Team 90 GHz (MALT90) survey aims to characterise the physical and ch...
The Millimetre Astronomy Legacy Team 90 GHz (MALT90) survey aims to characterise the physical and ch...
The Millimetre Astronomy Legacy Team 90 GHz (MALT90) survey aims to characterise the physical and ch...
We describe a pilot survey conducted with the Mopra 22 m radio telescope in preparation for the Mill...
ALMA will revolutionize our understanding of star formation within our galaxy, but before we can use...
The Millimetre Astronomy Legacy Team 90 GHz survey aims to characterise the physical and chemical ev...
textMassive stars play a key role in the evolution of the Galaxy; hence they are important objects o...
This thesis focuses on high-mass star formation by using infrared and sub-millimeter data mainly fro...
We introduce the Millimetre Astronomer's Legacy Team - 45 GHz (MALT-45) Galactic plane survey and de...
We present the current status of the SuperMALT, a follow up of the MALT90 project which obser...
We introduce the Millimetre Astronomer's Legacy Team – 45 GHz (MALT-45) Galactic plane survey and de...
We present the first results from the MALT-45 (Millimetre Astronomer's Legacy Team-45 GHz) Galactic ...
I studied the formation of massive stars and clusters via millimeter, radio, and infrared observatio...
We characterise the Millimetre Astronomy Legacy Team 90 GHz Survey (MALT90) and the Mopra telescope ...
We report Atacama Large Millimeter Array observations of 3 mm dust continuum emission and line emiss...
The Millimetre Astronomy Legacy Team 90 GHz (MALT90) survey aims to characterise the physical and ch...
The Millimetre Astronomy Legacy Team 90 GHz (MALT90) survey aims to characterise the physical and ch...
The Millimetre Astronomy Legacy Team 90 GHz (MALT90) survey aims to characterise the physical and ch...
We describe a pilot survey conducted with the Mopra 22 m radio telescope in preparation for the Mill...
ALMA will revolutionize our understanding of star formation within our galaxy, but before we can use...
The Millimetre Astronomy Legacy Team 90 GHz survey aims to characterise the physical and chemical ev...
textMassive stars play a key role in the evolution of the Galaxy; hence they are important objects o...
This thesis focuses on high-mass star formation by using infrared and sub-millimeter data mainly fro...
We introduce the Millimetre Astronomer's Legacy Team - 45 GHz (MALT-45) Galactic plane survey and de...
We present the current status of the SuperMALT, a follow up of the MALT90 project which obser...
We introduce the Millimetre Astronomer's Legacy Team – 45 GHz (MALT-45) Galactic plane survey and de...
We present the first results from the MALT-45 (Millimetre Astronomer's Legacy Team-45 GHz) Galactic ...
I studied the formation of massive stars and clusters via millimeter, radio, and infrared observatio...
We characterise the Millimetre Astronomy Legacy Team 90 GHz Survey (MALT90) and the Mopra telescope ...
We report Atacama Large Millimeter Array observations of 3 mm dust continuum emission and line emiss...