The JCMT Gould Belt Survey : SCUBA-2 observations of radiative feedback in NGC 1333

From National Research Council Canada

Download
  1. (PDF, 819 KB)
DOIResolve DOI: https://doi.org/10.1093/mnrasl/sls015
AuthorSearch for: ; Search for: ; Search for: ; Search for: ; Search for: ; Search for: ; Search for: 1; Search for:
Name affiliation
  1. National Research Council Canada. Herzberg Astronomy and Astrophysics
FormatText
TypeArticle
Journal titleMonthly Notices of the Royal Astronomical Society: Letters
ISSN1745-3925
1745-3933
Volume429
Issue1
PagesL10–L14
Subjectstars: formation; dust; extinction; submillimetre: ISM; stars: protostars
Abstract
We present observations of NGC 1333 from SCUBA-2 on the James Clerk Maxwell Telescope (JCMT), observed as a JCMT Gould Belt Survey pilot project during the shared risk campaign when the first of four arrays was installed at each of 450 and 850 μm. Temperature maps are derived from 450 and 850 μm ratios under the assumption of constant dust opacity spectral index β = 1.8. Temperatures indicate that the dust in the northern (IRAS 6/8) region of NGC 1333 is hot, 20–40 K, due to heating by the B star SVS3, other young stars in the IR/optically visible cluster and embedded protostars. Other luminous protostars are also identified by temperature rises at the 17 arcsec resolution of the ratio maps (0.02 pc assuming a distance of 250 pc for Perseus). The extensive heating raises the possibility that the radiative feedback may lead to increased masses for the next generation of stars.
Publication date
PublisherThe authors on behalf of the JCMT GBS Consortium (Oxford)
LanguageEnglish
Peer reviewedYes
NPARC number23001799
Export citationExport as RIS
Report a correctionReport a correction
Record identifier20ef263d-6b06-4e58-bff9-df04444e7a41
Record created2017-04-07
Record modified2020-02-06
Report a problem on this page
Date modified: