Thermal emission from cold dust grains in giant molecular clouds can be used to probe the physical properties, such as density, temperature and emissivity in star-forming regions. We present the Submillimetre Common-User Bolometer Array (SCUBA-2) shared-risk observations at 450 and 850 μm of the Orion A molecular cloud complex taken at the James Clerk Maxwell Telescope (JCMT). Previous studies showed that molecular emission lines can contribute significantly to the measured fluxes in those continuum bands. We use the Heterodyne Array Receiver Programme 12CO J = 3-2 integrated intensity map for Orion A in order to evaluate the molecular line contamination and its effects on the SCUBA-2 maps. With the corrected fluxes, we have obtained a new ...
This is the final version of the article. Available from OUP via the DOI in this record.Observations...
We present a new 3.3 mm continuum map of the Orion Molecular Cloud (OMC) 2/3 region. When paired wit...
We present the JCMT Gould Belt Survey's first look results of the southern extent of the Orion A Mol...
Thermal emission from cold dust grains in giant molecular clouds can be used to probe the physical p...
The emissivity spectral index is a critical component in the study of the physical properties of dus...
Observations of the dust emission using millimetre/submillimetre bolometer arrays can be contaminate...
The Gould Belt Legacy Survey will map star-forming regions within 500 pc, using HARP (Heterodyne Arr...
Observations of the dust emission using millimetre/submillimetre bolometer arrays can be contaminate...
The Gould Belt Legacy Survey will map star-forming regions within 500 pc, using Heterodyne Array Rec...
The Gould Belt Legacy Survey will map star-forming regions within 500pc, using Heterodyne Array Rece...
The Gould Belt Legacy Survey will map star-forming regions within 500 pc, using Heterodyne Array Rec...
International audienceContext. The [C II] 158 μm fine-structure line is the dominant cooling line of...
We present the JCMT Gould Belt Survey’s first look results of the southern extent of the Orion A Mol...
We present SCUBA-2 450 μm and 850 μm observations of the W40 complex in the Serpens- Aquila region a...
We present SCUBA-2 450 μm and 850 μm observations of the W40 complex in the Serpens-Aquila region as...
This is the final version of the article. Available from OUP via the DOI in this record.Observations...
We present a new 3.3 mm continuum map of the Orion Molecular Cloud (OMC) 2/3 region. When paired wit...
We present the JCMT Gould Belt Survey's first look results of the southern extent of the Orion A Mol...
Thermal emission from cold dust grains in giant molecular clouds can be used to probe the physical p...
The emissivity spectral index is a critical component in the study of the physical properties of dus...
Observations of the dust emission using millimetre/submillimetre bolometer arrays can be contaminate...
The Gould Belt Legacy Survey will map star-forming regions within 500 pc, using HARP (Heterodyne Arr...
Observations of the dust emission using millimetre/submillimetre bolometer arrays can be contaminate...
The Gould Belt Legacy Survey will map star-forming regions within 500 pc, using Heterodyne Array Rec...
The Gould Belt Legacy Survey will map star-forming regions within 500pc, using Heterodyne Array Rece...
The Gould Belt Legacy Survey will map star-forming regions within 500 pc, using Heterodyne Array Rec...
International audienceContext. The [C II] 158 μm fine-structure line is the dominant cooling line of...
We present the JCMT Gould Belt Survey’s first look results of the southern extent of the Orion A Mol...
We present SCUBA-2 450 μm and 850 μm observations of the W40 complex in the Serpens- Aquila region a...
We present SCUBA-2 450 μm and 850 μm observations of the W40 complex in the Serpens-Aquila region as...
This is the final version of the article. Available from OUP via the DOI in this record.Observations...
We present a new 3.3 mm continuum map of the Orion Molecular Cloud (OMC) 2/3 region. When paired wit...
We present the JCMT Gould Belt Survey's first look results of the southern extent of the Orion A Mol...