Browsing by Author "Moore, T.J.T."

Now showing items 1-14 of 14

    • ATLASGAL - environments of 6.7 GHz methanol masers 

      Urquhart, J.S.; Moore, T.J.T.; Schuller, F.; Wyrowski, F.; Menten, K. M.; Thompson, M. A.; Csengeri, T.; Walmsley, C.M.; Bronfman, L.; König, C. (2013-05-01)
      Using the 870 micron APEX Telescope large area survey of the Galaxy, we have identified 577 submillimetre continuum sources with masers from the methanol multibeam survey in the region 280deg lt ell lt 20deg; |b| lt 1deg.5 ...

    • CHIMPS: the 13CO/C18O (J = 3 to 2) Heterodyne Inner Milky Way Plane Survey 

      Rigby, A.J.; Moore, T.J.T.; Plume, R.; Eden, D.J.; Urquhart, J.S.; Thompson, M.A.; Mottram, J.C.; Brunt, C.M.; Butner, H. M.; Dempsey, J. T.; Gibson, S.J.; Hatchell, J.; Jenness, T.; Kuno, N.; Longmore, S.N.; Morgan, L.K.; Polychroni, D.; Thomas, H.; White, G.J.; Zhu, M. (2016-03-01)
      We present the 13CO/C18O (J = 3 → 2) Heterodyne Inner Milky Way Plane Survey (CHIMPS) which has been carried out using the Heterodyne Array Receiver Program on the 15 m James Clerk Maxwell Telescope (JCMT) in Hawaii. The ...

    • The Coordinated Radio and Infrared Survey for High-Mass Star Formation (The CORNISH Survey). I : Survey Design 

      Hoare, M.G.; Purcell, C.R.; Churchwell, E.B.; Diamond, P.; Cotton, W.D.; Chandler, C.J.; Smethurst, S.; Kurtz, S.E.; Mundy, L.G.; Dougherty, S.M.; Fender, R.P.; Fuller, G.A.; Jackson, J.M.; Garrington, S.T.; Gledhill, T.; Goldsmith, P.F.; Lumsden, S.L.; Martí, J.; Moore, T.J.T.; Muxlow, T.W.B.; Oudmaijer, R.D.; Pandian, J.D.; Paredes, J.M.; Shepherd, D.S.; Spencer, R.E.; Thompson, M.A.; Umana, G.; Urquhart, J.S.; Zijlstra, A.A. (2012-09-01)
      We describe the motivation, design, and implementation of the CORNISH survey, an arcsecond-resolution radio continuum survey of the inner galactic plane at 5 GHz using the Very Large Array (VLA). It is a blind survey ...

    • The Coordinated Radio and Infrared Survey for High-mass Star Formation II : Source Catalog 

      Purcell, C.R.; Hoare, M.G.; Cotton, W.D.; Lumsden, S. L.; Urquhart, J.S.; Chandler, C.; Churchwell, E.B.; Diamond, P.; Dougherty, S.M.; Fender, R.P.; Fuller, G.; Garrington, S.T.; Gledhill, T.; Goldsmith, P.F.; Hindson, L.; Jackson, J.M.; Kurtz, S.E.; Martí, J.; Moore, T.J.T.; Mundy, L.G.; Muxlow, T.W.B.; Oudmaijer, R.D.; Pandian, J.D.; Paredes, J.M.; Shepherd, D.S.; Smethurst, S.; Spencer, R.E.; Thompson, M.A.; Umana, G.; Zijlstra, A.A. (2013-03-01)
      The CORNISH project is the highest resolution radio continuum survey of the Galactic plane to date. It is the 5 GHz radio continuum part of a series of multi-wavelength surveys that focus on the northern GLIMPSE region ...

    • The effect of spiral arms on star formation in the Galaxy 

      Moore, T.J.T.; Urquhart, J.S.; Morgan, L.K.; Thompson, M.A. (2012-10-11)

    • Geometric configuration around GL 2591 : an infrared reflection nebula and a CS molecular disk 

      Yamashita, T.; Sato, S.; Tamura, M.; Suzuki, H.; Kaifu, N.; Takano, T.; Mountain, C.M.; Moore, T.J.T.; Gatley, I.; Hough, J. (1987)

    • Giving physical significance to the Hi-GAL data : determining the distance of cold dusty cores in the Milky Way 

      Russeil, D.; Pestalozzi, M.; Mottram, J.C.; Bontemps, S.; Anderson, L.D.; Zavagno, A.; Beltran, M.T.; Bally, J.; Brand, J.; Brunt, C.; Cesaroni, R.; Joncas, G.; Marshall, D.; Martin, P.; Massi, F.; Molinari, S.; Moore, T.J.T.; Noriega-Crespo, A.; Olmi, L.; Thompson, M.A.; Wienen, M.; Wyrowski, F. (2011)
      Context: Hi-GAL, an open time key-project of the Herschel satellite, was awarded 343 hours observing time to carry out a 5-band photometric imaging survey at 70, 160, 250, 350, and 500 mu m of a vertical bar b vertical bar ...

    • Infrared polarimetry of the southern massive star-forming region G333.6-0.2 

      Fujiyoshi, T.; Smith, C.H.; Wright, C.M.; Moore, T.J.T.; Aitken, D.; Roche, P.F. (2001)
      We present 8-13μm spectropolarimetry, and 12- and 2-μm imaging polarimetry of the southern massive star-forming region G333.6−0.2. Spectro-polarimetry measurements show that the polarization observed towards the nebula ...

    • Infrared reflection nebula in W75N 

      Yamashita, T.; Sato, S.; Tamura, M.; Suzuki, H.; Gatley, I.; Hough, J.; Mountain, C.M.; Moore, T.J.T. (1988)
      A new infrared reflection nebula is identified in the W75N region. The K-band polarization map shows a centrosymmetric pattern of the vectors extending over a region 2 arcmin in size, with large values of degrees of ...

    • 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 ...

    • Near-infrared imaging observations of the southern massive star-forming region G333.6-0.2 

      Fujiyoshi, T.; Smith, C.H.; Moore, T.J.T.; Lumsden, S.; Aitken, D.; Roche, P.F. (2005)
      We present near-infrared broad-band JHK' images of the southern massive star-forming region G333.6−0.2. The slope of the K-luminosity function towards the region (0.24 ± 0.01) is considered to be equivalent to that expected ...

    • Radio and infrared recombination studies of the southern massive star forming region G333.6-0.2 

      Fujiyoshi, T.; Smith, C.H.; Caswell, J.L.; Moore, T.J.T.; Lumsden, S.; Aitken, D.; Roche, P.F. (2006)

    • Star formation in Galactic spiral arms and the interarm regions 

      Eden, D.J.; Moore, T.J.T.; Morgan, L.K.; Thompson, M.A.; Urquhart, J.S. (2013-05-11)
      The line of sight through the Galactic plane between longitudes l = 37deg.83 and 42deg.50 allows for the separation of Galactic Ring Survey molecular clouds into those that fall within the spiral arms and those located in ...

    • The statistics of triggered star formation : an overdensity of massive young stellar objects around Spitzer bubbles 

      Thompson, Mark; Urquhart, J.S.; Moore, T.J.T.; Morgan, L.K. (2012-03-01)
      We present a detailed statistical study of massive star formation in the environment of 322 Spitzer mid-infrared bubbles by using the Red MSX Source (RMS) survey for massive young stellar objects (YSOs). Using a combination ...