| 2nd of September 2015 |
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| ATNF Colloquium |
| Tightening the belt: Constraining the mass and evolution in SDC335 |
| by Adam Avison (University of Manchester) |
| ALMA Cycle 0 observations identified one of the most massive star-forming cores observed in the Milky Way. Situated within the IRDC SDC335.579-0.292 this core, along with an accompanying lower mass core, appear to be in the early stages of forming massive (M*
> 8 Msolar) stars. In this talk the results of ATCA follow up continuum observations (6, 8, 23, 25 GHz) will be presented. The results of which have allowed us to identify 3 hyper compact HII regions within SDC335 and characterise the protostars creating them. From these results we are able to put constraints on the future stellar population in SDC335. |