Staff profile
Dr Mark Swinbank
(email at a.m.swinbank@durham.ac.uk)
Research Groups
Publications
- 1: 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, K. E. K., 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). Intense star formation within resolved compact regions in a galaxy at z = 2.3. Nature 464(7289): 733-736.
- 2: Swinbank, A. M., Smail, Ian, Chapman, S. C., Borys, C., Alexander, D. M., Blain, A. W., Conselice, C. J., Hainline, L. J. & Ivison, R. J. (2010). A Hubble Space Telescope NICMOS and ACS morphological study of z∼ 2 submillimetre galaxies. Monthly Notices of the Royal Astronomical Society 405(1): 234-244.
- 4: Swinbank, A.M., Papadopoulos, P.P., Cox, P., Krips, M., Ivison, R.J., Smail, Ian, Thomson, A.P., Neri, R., Richard, J. & Ebeling, H. (2011). The Interstellar Medium in Distant Star-forming Galaxies: Turbulent Pressure, Fragmentation, and Cloud Scaling Relations in a Dense Gas Disk at z = 2.3. The Astrophysical Journal 742(1): 11.
- 5: Swinbank, A. M., Smail, Ian, Sobral, D., Theuns, T., Best, P. N. & Geach, J. E. (2012). The Properties of the Star-Forming Interstellar Medium at z=0.84-2.23 from HiZELS II: Star-Formation and Clump Scaling Laws in Gas Rich, Turbulent Disks. THE ASTROPHYSICAL JOURNAL 760(2): 130.
- 6: Swinbank, A. M., Sobral, D., Smail, Ian, Geach, J. E., Best, P. N., McCarthy, I. G., Crain, R. A. & Theuns, T. (2012). The properties of the star-forming interstellar medium at z=0.84-2.23 from HiZELS: mapping the internal dynamics and metallicity gradients in high-redshift disc galaxies. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 426(2): 935-950.
- 7: Swinbank, A. M., Lacey, C. G., Smail, Ian, Baugh, C. M., Frenk, C. S., Blain, A. W., Chapman, S. C., Coppin, K. E. K., Ivison, R. J., Gonzalez, J. E. & Hainline, L. J. (2008). The properties of submm galaxies in hierarchical models. Monthly Notices of the Royal Astronomical Society 391(1): 420-434.