A search for outflows towards massive YSO disk candidates

Computer Science

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Galactic, Mopra

Scientific paper

We intend to search for outflows towards a selection of candidate massive YSO disks. This proposal is a companion to C1801, which seeks to identify the disks through NH3 (4,4) and (5,5) emission. We will use Mopra to create OTF maps around seven of these candidates in multiple spectral lines. We will focus our efforts on SiO, HCO+, CS, HCN and HNC, most of which show evidence for outflow wings in their spectra. The molecular outflows are important complementary information for the disk studies because outflows need to be oriented perpendicular to the accretion disks. These observations will reveal the outflow axis, masses and energetics, which are important input parameters to characterize the source properties in relation with the underlying accretion disks.

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