Browsing by Author "Hogerheijde, M.R."

Now showing items 1-5 of 5

    • The James Clerk Maxwell Telescope Legacy Survey of Nearby Star-forming Regions in the Gould Belt 

      Ward-Thompson, D.; Di Francesco, J.; Hatchell, J.; Hogerheijde, M.R.; Nutter, D.; Bastien, P.; Basu, S.; Bonnell, I.; Bowey, J.; Brunt, C.; Buckle, J.; Butner, H.; Cavanagh, B.; Chrysostomou, A. (2007)
      This paper describes a James Clerk Maxwell Telescope (JCMT) legacy survey that has been awarded roughly 500 hr of observing time to be carried out from 2007 to 2009. In this survey, we will map with SCUBA-2 (Submillimetre ...

    • The James Clerk Maxwell Telescope Spectral Legacy Survey 

      Plume, R.; Fuller, G.A.; Helmich, F.; van der Tak, F.F.S.; Roberts, H.; Bowey, J.; Buckle, J.; Butner, H.; Caux, E.; Ceccarelli, C.; van Dishoeck, E.F.; Friberg, P.; Gibb, A.G.; Hatchell, J.; Hogerheijde, M.R.; Matthews, H.; Millar, T.J.; Mitchell, G.; Moore, T.J.T.; Ossenkopf, V.; Rawlings, J.M.C.; Richer, J.; Roellig, M.; Schilke, P.; Spaans, M.; Tielens, A.G.G.M.; Thompson, M.A.; Viti, S.; Weferling, B.; White, G.J.; Wouterloot, J.; Yates, J.A.; Zhu, M. (2007)
      Stars form in the densest, coldest, most quiescent regions of molecular clouds. Molecules provide the only probes that can reveal the dynamics, physics, chemistry, and evolution of these regions, but our understanding of ...

    • The JCMT Gould Belt survey : Evidence for radiative heating in serpens MWC 297 and its influence on local star formation 

      Rumble, D.; Hatchell, J.; Gutermuth, R. A.; Kirk, H.; Buckle, J.; Beaulieu, S. F.; Berry, D.S.; Broekhoven-Fiene, H.; Currie, M. J.; Fich, M.; Jenness, T.; Johnstone, D.; Mottram, J. C.; Nutter, D.; Pattle, K.; Pineda, J. E.; Quinn, C.; Salji, C.; Tisi, S.; Walker-Smith, S.; Di Francesco, J.; Hogerheijde, M.R.; Ward-Thompson, D.; Allen, L.E.; Cieza, L. A.; Dunham, M. M.; Harvey, P. M.; Stapelfeldt, K. R.; Bastien, P.; Butner, H.; Chen, M.; Chrysostomou, A.; Coude, S.; Davis, C.J.; Drabek-Maunder, E.; Duarte-Cabral, A.; Fiege, J.; Friberg, P.; Friesen, R.; Fuller, G.A.; Graves, S.; Greaves, J.; Gregson, J.; Holland, W.; Joncas, G.; Kirk, J.M.; Knee, L. B. G.; Mairs, S.; Marsh, K.; Matthews, B. C.; Moriarty-Schieven, G.; Rawlings, J.; Richer, J.; Robertson, D.; Rosolowsky, E.; Sadavoy, S.; Thomas, H.; Tothill, N.; Viti, S.; White, G.J.; Wilson, C. D.; Wouterloot, J.; Yates, J.; Zhu, M. (2015-04-01)
      We present SCUBA-2 450 and 850 μm observations of the Serpens MWC 297 region, part of the James Clerk Maxwell Telescope (JCMT) Gould Belt Survey of nearby star-forming regions. Simulations suggest that radiative feedback ...

    • The JCMT Legacy Survey of the Gould Belt : mapping 13CO and C18O in Orion A 

      Buckle, J. V.; Davis, C.J.; Di Francesco, J.; Graves, S. F.; Nutter, D.; Richer, J. S.; Roberts, J. F.; Ward-Thompson, D.; White, G.J.; Brunt, C.; Butner, H. M.; Cavanagh, B.; Chrysostomou, A.; Curtis, E.I.; Duarte-Cabral, A.; Etxaluze, M.; Fich, M.; Friberg, P.; Friesen, R.; Fuller, G.A.; Greaves, J.S.; Hatchell, J.; Hogerheijde, M.R.; Johnstone, D.; Matthews, B.; Matthews, H.; Rawlings, J.M.C.; Sadavoy, S.; Simpson, R.J.; Tothill, N.F.H.; Tsamis, Y.G.; Viti, S.; Wouterloot, J. G. A.; Yates, J. (2012-05)
      The Gould Belt Legacy Survey will map star-forming regions within 500 pc, using Heterodyne Array Receiver Programme (HARP), Submillimetre Common-User Bolometer Array 2 (SCUBA-2) and Polarimeter 2 (POL-2) on the James Clerk ...

    • The JCMT Legacy Survey of the Gould Belt: a first look at Orion B with HARP 

      Buckle, J.; Curtis, E.I.; Roberts, J.F.; White, G.J.; Hatchell, J.; Brunt, C.; Butner, H.; Cavanagh, B.; Chrysostomou, A.; Davis, C.J.; Duarte-Cabral, A.; Etxaluze, M.; Di Francesco, J.; Friberg, P.; Friesen, R.; Fuller, G.A.; Graves, S.; Greaves, J.S.; Hogerheijde, M.R.; Johnstone, D.; Matthews, B.; Matthews, H.; Nutter, D.; Rawlings, J.M.C.; Richer, J.; Sadavoy, S.; Simpson, R.J.; Tothill, N.F.H.; Tsamis, Y.G.; Viti, S.; Ward-Thompson, D.; Wouterloot, J.; Yates, J.A. (2010)
      The Gould Belt Legacy Survey will survey nearby star-forming regions (within 500 pc), using Heterodyne Array Receiver Programme (HARP), Submillimetre Common-User Bolometer Array 2 and Polarimeter 2 on the James Clerk Maxwell ...