The JCMT Gould Belt Survey: low-mass protoplanetary discs from a SCUBA-2 census of NGC 1333

P. Dodds, J. S. Greaves, A. Scholz, J. Hatchell, W. S. Holland, JCMT Gould Belt Survey Team

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9 Citations (Scopus)

Abstract

NGC 1333 is a 1–2 Myr old cluster of stars in the Perseus molecular cloud. We used 850 μm data from the Gould Belt Survey with SCUBA-2 on the James Clerk Maxwell Telescope to measure or place limits on disc masses for 82 Class II sources in this cluster. Eight disc candidates were detected; one is estimated to have mass of about 9 MJup in dust plus gas, while the others host only 2–4 MJup of circumstellar material. None of these discs exceeds the threshold for the ‘minimum mass solar nebula’ (MMSN). This reinforces previous claims that only a small fraction of Class II sources at an age of 1–2 Myr have discs exceeding the MMSN threshold and thus can form a planetary system like our own. However, other regions with similarly low fractions of MMSN discs (IC 348, UpSco, σ Ori) are thought to be older than NGC 1333. Compared with coeval regions, the exceptionally low fraction of massive discs in NGC 1333 cannot easily be explained by the effects of UV radiation or stellar encounters. Our results indicate that additional environmental factors significantly affect disc evolution and the outcome of planet formation by core accretion.

Original languageEnglish
Pages (from-to)722-727
JournalMonthly Notices of the Royal Astronomical Society
Volume447
Issue number1
Early online date19 Dec 2014
DOIs
Publication statusPublished - 11 Feb 2015

Keywords

  • Planets and satellites: formation
  • Protoplanetary discs
  • Stars: formation
  • Stars: pre-main-sequence

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