Description
This dataset contains synthetic 1.3mm dust continuum images of massive protoclusters which are generated using analytic models and radiative transfer calculations. The images are used to investigate the observability of low-mass cores in massive protoclusters. The data category is organised in a hierarchical way: separation, mass of high-mass star, mass of low-mass star, resolution. All the images are in .FITS format, which can be viewed using DS9 or CASA/CARTA.
| Date made available | 22 Sept 2023 |
|---|---|
| Publisher | University of St Andrews |
| Date of data production | 1 May 2021 - 1 May 2022 |
Student theses
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The formation of high-mass stars and stellar clusters
Zhang, S. (Author), Cyganowski, C. J. (Supervisor) & Bonnell, I. A. (Supervisor), 29 Nov 2023Student thesis: Doctoral Thesis (PhD)