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SUMMARY:The JCMT Gould Belt Survey – Results from HARP and SCUBA-2 - Sam
 antha Walker-Smith (Cavendish Astrophysics)
DTSTART:20131119T170000Z
DTEND:20131119T173000Z
UID:TALK47330@talks.cam.ac.uk
CONTACT:David Titterington
DESCRIPTION:The Gould Belt Survey is a project to map a large number of ne
 arby star-forming molecular clouds\, and includes a range of environments 
 – from the energetic clustered Orion cloud to the low-mass cool Taurus c
 loud.  It will use HARP and SCUBA-2 to make velocity-resolved measurements
  of molecular gas and to map the dust continuum respectively.\n\nI will pr
 esent some new SCUBA-2 data that I have reduced\, as an example of the fin
 ished maps that we produce.  I will also present a comparison on HCO+ and 
 HCN emission\, which traces the dense gas in star-forming regions.\n
LOCATION:Martin Ryle Seminar Room\, Kavli Institute
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