2013MNRAS.435.1671W
A SCUBA-2 850-μm survey of protoplanetary discs in the σ Orionis cluster
Williams, Jonathan P. ( Institute for Astronomy, University of Hawaii at Manoa, Honolulu, HI 96822, USA; ); Cieza, Lucas A. ( Institute for Astronomy, University of Hawaii at Manoa, Honolulu, HI 96822, USA; Universidad Diego Portales, Facultad de Ingeniería, Av. Ejército 441, Santiago, Chile ); Andrews, Sean M. ( Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA ); Coulson, Iain M. ( Joint Astronomy Centre, 660 N. A`ohk Place, University Park, Hilo, HI 96720, USA ); Barger, Amy J. ( Institute for Astronomy, University of Hawaii at Manoa, Honolulu, HI 96822, USA; Department of Astronomy, University of Wisconsin-Madison, 475 North Charter Street, Madison, WI 53706, USA; Department of Physics and Astronomy, University of Hawaii, 2505 Correa Road, Honolulu, HI 96822, USA ); Casey, Caitlin M. ( Institute for Astronomy, University of Hawaii at Manoa, Honolulu, HI 96822, USA ); Chen, Chian-Chou ( Institute for Astronomy, University of Hawaii at Manoa, Honolulu, HI 96822, USA ); Cowie, Lennox L. ( Institute for Astronomy, University of Hawaii at Manoa, Honolulu, HI 96822, USA ); Koss, Michael ( Institute for Astronomy, University of Hawaii at Manoa, Honolulu, HI 96822, USA ); Lee, Nicholas ( Institute for Astronomy, University of Hawaii at Manoa, Honolulu, HI 96822, USA ); Sanders, David B. ( Institute for Astronomy, University of Hawaii at Manoa, Honolulu, HI 96822, USA ) and 1 coauthors show affiliations
Monthly Notices of the Royal Astronomical Society, Volume 435, Issue 2, p.1671-1679
Published in Oct 2013
We present the results from a large 850-μm survey of the σ Orionis cluster using the SCUBA-2 camera on the James Clerk Maxwell Telescope. The 0.5° diameter circular region we surveyed contains 297 young stellar objects with an age estimated at about 3 Myr. We detect nine of these objects, eight of which have infrared excesses from an inner disc. We also serendipitously detect three non-stellar sources at >5σ that are likely background submillimetre galaxies. The nine detected stars have inferred disc masses ranging from 5 to about 17 MJup, assuming similar dust properties as Taurus discs and an interstellar medium gas-to-dust ratio of 100. There is a net positive signal towards the positions of the individually undetected infrared excess sources indicating a mean disc mass of 0.5 MJup. Stacking the emission towards those stars without infrared excesses constrains their mean disc mass to less than 0.3 MJup, or an equivalent Earth mass in dust. The submillimetre luminosity distribution is significantly different from that in the younger Taurus region, indicating disc mass evolution as star-forming regions age and the infrared excess fraction decreases. Submillimetre Array observations reveal CO emission towards four sources demonstrating that some, but probably not much, molecular gas remains in these relatively evolved discs. These observations provide new constraints on the dust and gas mass of protoplanetary discs during the giant planet building phase and provide a reference level for future studies of disc evolution.
Keywords:
Astronomy: protoplanetary discs; submillimetre: stars
arXiv: Astrophysics - Earth and Planetary Astrophysics; Astrophysics - Galaxy Astrophysics; Astrophysics - Solar and Stellar Astrophysics
2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
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