|COOKIES: By using this website you agree that we can place Google Analytics Cookies on your device for performance monitoring.|
The JCMT Gould Belt Survey – Results from HARP and SCUBA-2
If you have a question about this talk, please contact David Titterington.
The Gould Belt Survey is a project to map a large number of nearby star-forming molecular clouds, and includes a range of environments – from the energetic clustered Orion cloud to the low-mass cool Taurus cloud. It will use HARP and SCUBA -2 to make velocity-resolved measurements of molecular gas and to map the dust continuum respectively.
I will present some new SCUBA -2 data that I have reduced, as an example of the finished maps that we produce. I will also present a comparison on HCO + and HCN emission, which traces the dense gas in star-forming regions.
This talk is part of the Cavendish Astrophysics Seminars series.
This talk is included in these lists:
Note that ex-directory lists are not shown.
Other listsDivision F Financial Modelling Group Cambridge University Anthropological Society Trinity Mathematical Society
Other talksApplying adjoint methods to the glacial isostatic adjustment inverse problem Review Talk: SUSY breaking in realistic model building What Biologists can learn from bats Floral quartets link flower development and evolution The Lyrical in Epic Time: On Modern Chinese Literary Thought Insect biodiversity in Cambridge – rare species in our urban meadows