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A deeply embedded young protoplanetary disk around L1489 IRS observed by the submillimeter array
C. Brinch, A. Crapsi, J. K. Jorgensen +2
Circumstellar disks are expected to form early in the process that leads to the formation of a young star, during the collapse of the dense molecular cloud core. It is currently no…
Profiling Young Massive Stars
T. Hill, M. G. Burton, M. R. Cunningham +1
We present the results of spectral energy distribution analysis for 162 of the 405 sources reported in the SIMBA survey of Hill et al. (2005). The fits reveal source specific param…
A Search for Propylene Oxide and Glycine in Sagittarius B2 (LMH) and Orion
M. R. Cunningham, P. A. Jones, P. D. Godfrey +17
We have used the Mopra Telescope to search for glycine and the simple chiral molecule propylene oxide in the Sgr B2 (LMH) and Orion KL, in the 3-mm band. We have not detected eithe…
Millimetre Continuum Observations of Southern Massive Star Formation Regions II. SCUBA observations of cold cores and the dust grain emissivity index
T. Hill, M. A. Thompson, M. G. Burton +4
We report the results of a submillimetre continuum emission survey targeted toward 78 star formation regions, 72 of which are devoid of methanol maser and UC HII regions, identifie…
A CH3CN and HCO+ survey towards southern methanol masers associated with star formation
C. R. Purcell, R. Balasubramanyam, M. G. Burton +32
We present the initial results of a 3-mm spectral line survey towards 83 methanol maser selected massive star-forming regions. Here we report observations of the J=5-4 and 6-5 rota…
Millimetre continuum observations of southern massive star formation regions. I. SIMBA observations of cold cores
T. Hill, M. G. Burton, V. Minier +4
We report the results of a SEST 1.2 mm continuum emission survey toward regions previously identified as harbouring a methanol maser and/or an UC HII region, typically indicative o…
High-mass star formation in the Southern Hemisphere sky
V. Minier, M. G. Burton, T. Hill +4
We report on a multi-wavelength (IR to cm) and multi-resolution (1 mas to 20 arcsec) exploration of high-mass star formation regions in the Galactic plane, at longitudes observable…