This paper presents observations of the Lupus I molecular cloud at 450 and 850 mum with Submillimetre Common User Bolometer Array (SCUBA-2) as part of the James Clerk Maxwell Telescope Gould Belt Survey (JCMT GBS). Nine compact sources, assumed to be the discs of young stellar objects (YSOs), 12 extended protostellar, pre-stellar and starless cores, and one isolated, low-luminosity protostar, are detected in the region. Spectral energy distributions, including submillimetre fluxes, are produced for 15 YSOs, and each is fitted with the models of Robitaille et al. The proportion of Class 0/I protostars is higher than that seen in other Gould Belt regions such as Ophiuchus and Serpens. Circumstellar disc masses are calculated for more evolved ...
We present 850 and 450 mu m observations of the dense regions within the Auriga-California molecular...
This thesis presents my work characterising star formation in Gould Belt molecular clouds using subm...
In this paper, we present the first observations of the Ophiuchus molecular cloud performed as part ...
This paper presents observations of the Lupus I molecular cloud at 450 and 850 μm with Submillimetre...
This paper presents observations of the Lupus I molecular cloud at 450 and 850 μm with Submillimetr...
This paper presents observations of the Lupus I molecular cloud at 450 and 850 μm with Submillimetr...
This paper presents observations of the Lupus I molecular cloud at 450 and 850 μm with Submillimetre...
This paper presents observations of the Lupus I molecular cloud at 450 and 850 μm with Submillimetre...
This paper presents observations of the Lupus I molecular cloud at 450 and 850 μm with Submillimetre...
This paper presents observations of the Lupus I molecular cloud at 450 and 850 μm with Submillimetre...
This paper presents observations of the Lupus I molecular cloud at 450 and 850 μm with Submillimetre...
This is the final version of the article. Available from OUP via the DOI in this record.This paper p...
We present observations of the Cepheus Flare obtained as part of the James Clerk Maxwell Telescope (...
We present observations of the Cepheus Flare obtained as part of the James Clerk Maxwell Telescope (...
Context. How the diffuse medium of molecular clouds condenses in dense cores and how many of these c...
We present 850 and 450 mu m observations of the dense regions within the Auriga-California molecular...
This thesis presents my work characterising star formation in Gould Belt molecular clouds using subm...
In this paper, we present the first observations of the Ophiuchus molecular cloud performed as part ...
This paper presents observations of the Lupus I molecular cloud at 450 and 850 μm with Submillimetre...
This paper presents observations of the Lupus I molecular cloud at 450 and 850 μm with Submillimetr...
This paper presents observations of the Lupus I molecular cloud at 450 and 850 μm with Submillimetr...
This paper presents observations of the Lupus I molecular cloud at 450 and 850 μm with Submillimetre...
This paper presents observations of the Lupus I molecular cloud at 450 and 850 μm with Submillimetre...
This paper presents observations of the Lupus I molecular cloud at 450 and 850 μm with Submillimetre...
This paper presents observations of the Lupus I molecular cloud at 450 and 850 μm with Submillimetre...
This paper presents observations of the Lupus I molecular cloud at 450 and 850 μm with Submillimetre...
This is the final version of the article. Available from OUP via the DOI in this record.This paper p...
We present observations of the Cepheus Flare obtained as part of the James Clerk Maxwell Telescope (...
We present observations of the Cepheus Flare obtained as part of the James Clerk Maxwell Telescope (...
Context. How the diffuse medium of molecular clouds condenses in dense cores and how many of these c...
We present 850 and 450 mu m observations of the dense regions within the Auriga-California molecular...
This thesis presents my work characterising star formation in Gould Belt molecular clouds using subm...
In this paper, we present the first observations of the Ophiuchus molecular cloud performed as part ...