Journal Article

Resolved images of self-gravitating circumstellar discs with ALMA

Peter Cossins, Giuseppe Lodato and Leonardo Testi

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 407, issue 1, pages 181-188
Published in print September 2010 | ISSN: 0035-8711
Published online August 2010 | e-ISSN: 1365-2966 | DOI:
Resolved images of self-gravitating circumstellar discs with ALMA

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In this paper, we present simulated observations of massive self-gravitating circumstellar discs using the Atacama Large Millimetre/sub-millimetre Array (ALMA). Using a smoothed particle hydrodynamics model of a 0.2-M disc orbiting a 1-M protostar, with a cooling model appropriate for discs at temperatures below ∼160 K and representative dust opacities, we have constructed maps of the expected emission at sub-mm wavelengths. We have then used the Common Astronomy Software Applications ALMA simulator to generate simulated images and visibilities with various array configurations and observation frequencies, taking into account the expected thermal noise and atmospheric opacities. We find that at 345 GHz (870 μm) spiral structures at a resolution of a few au should be readily detectable in approximately face-on discs out to distances of the Taurus-Auriga star-forming complex.

Keywords: accretion, accretion discs; gravitation; instabilities; circumstellar matter; stars: pre-main-sequence; submillimetre: stars

Journal Article.  5559 words.  Illustrated.

Subjects: Astronomy and Astrophysics

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