SCUBA Mapping of Outer Galaxy Protostellar Candidates
arXiv:0707.3312 · doi:10.1051/0004-6361:20077878
Abstract
We aim to study dust properties of massive star forming regions in the outer Galaxy, in a direction opposite to the Galactic center. We present observations of six outer Galaxy point sources IRAS 01045+6505, 01420+6401, 05271+3059, 05345+3556, 20222+3541 and 20406+4555, taken with the Submillimeter Common-User Bolometer Array (SCUBA) on the James Clerk Maxwell Telescope (JCMT) at 450 and 850 micron. Single temperature greybody models are fitted to the Spectral Energy Distribution of the detected sub-mm cores to derive dust temperature, dust emissivity index and optical depth at 250 micron. The observed radial intensity profiles of the sub-mm cores were fitted with power laws to derive the indices describing the density distribution. At a resolution of 15" all six IRAS point sources show multiple emission peaks. Only four out of fourteen detected sub-mm cores show associated mid-infrared emission. For the sub-mm cores we derive dust temperatures of 32+-5 K and dust emissivity indices between 0.9 and 2.5. The density profiles of the sub-mm cores can be fitted by a single power law distribution with indices -1.5+-0.3, with most cores showing an index of -1.5. This is consistent with most observations of massive star forming regions and supports predictions of models of star formation which consider non-thermal support against gravitational collapse.
Accepted for publication in Astronomy & Astrophysics
References in corpus (11)
- SCUBA: A common-user submillimetre camera operating on the James Clerk Maxwell Telescope
- High-Mass Proto-Stellar Candidates - II : Density structure from dust continuum and CS emission
- High-Mass Proto-Stellar Candidates - I : The Sample and Initial Results
- The Physical Conditions for Massive Star Formation: Dust Continuum Maps and Modeling
- Structure and Evolution of the Envelopes of Deeply Embedded Massive Young Stars
- Molecular gas in late-type galaxies
- A search for evolved dust in Herbig Ae stars
- Testing envelope models of young stellar objects with submillimeter continuum and molecular-line observation
- A Model for the Internal Structure of Molecular Cloud Cores
- Probing the Early Stages of Low-Mass Star Formation in LDN 1689N: Dust and Water in IRAS 16293-2422A, B, and E
- Lensing Properties of Cored Galaxy Models