Browsing by Author "Longmore, S."

Now showing items 1-7 of 7

    • Anatomy of the S255-S257 complex - triggered high-mass star formation 

      Minier, V.; Peretto, N.; Longmore, S.; Burton, M.; Cesaroni, R.; Goddi, C.; Pestalozzi, M.; Andre, P. (Cambridge University Press, 2007)
      We present a multi-wavelength (NIR to radio) and multi-scale (1 AU to 10 pc) study of the S255–S257 complex of young high-mass (proto)stars. The complex consists of two evolved HII regions and a molecular gas filament in ...

    • Cloud Structure of Galactic OB Cluster-forming Regions from Combining Ground- and Space-based Bolometric Observations 

      Lin, Y.; Liu, H.~B.; Li, D.; Zhang, Z.-Y.; Ginsburg, A.; Pineda, J.~E.; Qian, L.; Galván-Madrid, R.; McLeod, A.~F.; Rosolowsky, E.; Dale, James; Immer, K.; Koch, E.; Longmore, S.; Testi, L.; Walker, D (2016-09-01)
      We have developed an iterative procedure to systematically combine the millimeter and submillimeter images of OB cluster-forming molecular clouds, which were taken by ground-based (CSO, JCMT, APEX, and IRAM-30 m) and space ...

    • Dense gas in the Galactic central molecular zone is warm and heated by turbulence 

      Ginsburg, A.; Henkel, C.; Ao, Y.; Riquelme, D.; Kauffmann, J.; Pillai, T.; Mills, E.~A.~C.; Requena-Torres, M.~A.; Immer, K.; Testi, L.; Ott, J.; Bally, J.; Battersby, C.; Darling, J.; Aalto, S.; Stanke, T.; Kendrew, S.; Kruijssen, J.~M.~D.; Longmore, S.; Guesten, R.; Menten, K.~M.; Dale, James (2016-01-26)
      Context. The Galactic center is the closest region where we can study star formation under extreme physical conditions like those in high-redshift galaxies. Aims. We measure the temperature of the dense gas in the central ...

    • Intense star formation within resolved compact regions in a galaxy at z = 2.3 

      Swinbank, A.M.; Smail, I.; Longmore, S.; Harris, A.I.; Baker, A.J.; De Breuck, C.; Richard, J.; Edge, A.C.; Ivison, R.J.; Blundell, R.; Coppin, Kristen; Cox, P.; Gurwell, M.; Hainline, L.J.; Krips, M.; Lundgren, A.; Neri, R.; Siana, B.; Siringo, G.; Stark, D.P.; Wilner, D.; Younger, J.D. (2010-04-01)
      Massive galaxies in the early Universe have been shown to be forming stars at surprisingly high rates. Prominent examples are dust-obscured galaxies which are luminous when observed at sub-millimetre wavelengths and which ...

    • The ionised, radical and molecular Milky Way: spectroscopic surveys with the SKA 

      Thompson, M.; Beuther, H.; Dickinson, C.; MOttram, J.; Klaassen, P.; Ginsburg, A.; Longmore, S.; Remijan, A.; Menten, K.~M. (Inspire, 2014-12-01)
      The bandwith, sensitivity and sheer survey speed of the SKA offers unique potential for deep spectroscopic surveys of the Milky Way. Within the frequency bands available to the SKA lie many transitions that trace the ...

    • Star and Stellar Cluster Formation: ALMA-SKA Synergies 

      Forbrich, Jan; Rathbone, J.; Fuller, G.; Longmore, S.; Molinari, S. (2015-04)
      Over the next decade, observations conducted with ALMA and the SKA will reveal the process of mass assembly and accretion onto young stars and will be revolutionary for studies of star formation. Here we summarise the ...

    • Star-forming protoclusters associated with methanol masers 

      Minier, V.; Burton, M.; Hill, T.; Pestalozzi, M.; Purcell, C.; Garay, G.; Walsh, A.; Longmore, S. (2005)