Now showing items 1-3 of 3

    • G11.92-0.61 MM1 : a Keplerian disc around a massive young proto-O star 

      Ilee, J. D.; Cyganowski, C. J.; Nazari, P.; Hunter, T. R.; Brogan, C. L.; Forgan, D. H.; Zhang, Q. (2016-11-11) - Journal article
      The formation process of massive stars is not well understood, and advancement in our understanding benefits from high-resolution observations and modelling of the gas and dust surrounding individual high-mass (proto)stars. ...
    • The Herschel-ATLAS Data Release 1 – II. Multi-wavelength counterparts to submillimetre sources 

      Bourne, N.; Dunne, L.; Maddox, S. J.; Dye, S.; Furlanetto, C.; Hoyos, C.; Smith, D. J. B.; Eales, S.; Smith, M. W. L.; Valiante, E.; Alpaslan, M.; Andrae, E.; Baldry, I. K.; Cluver, M. E.; Cooray, A.; Driver, S. P.; Dunlop, J. S.; Grootes, M. W.; Ivison, R. J.; Jarrett, T. H.; Liske, J.; Madore, B. F.; Popescu, C. C.; Robotham, A. G.; Rowlands, K.; Seibert, M.; Thompson, M. A.; Tuffs, R. J.; Viaene, S.; Wright, A. H. (2016-10-21) - Journal article
      This paper is the second in a pair of papers presenting data release 1 (DR1) of the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS), the largest single open-time key project carried out with the Herschel Space ...
    • Self-gravitating disc candidates around massive young stars 

      Forgan, D. H.; Ilee, J. D.; Cyganowski, C. J.; Brogan, C. L.; Hunter, T. R. (2016-11-21) - Journal article
      There have been several recent detections of candidate Keplerian discs around massive young protostars. Given the relatively large disc-to-star mass ratios in these systems, and their young ages, it is worth investigating ...