Now showing items 1-5 of 5

    • Accretion discs as regulators of stellar angular momentum evolution in the ONC and Taurus-Auriga 

      Davies, Claire; Gregory, Scott; Greaves, Jane Sophia (2014-10-21) - Journal article
      In light of recent substantial updates to spectral type estimations and newly established intrinsic colours, effective temperatures, and bolometric corrections for pre-main sequence (PMS) stars, we re-address the theory ...
    • Classical T Tauri stars : magnetic fields, coronae, and star-disc interactions 

      Johnstone, C. P.; Jardine, Moira Mary; Gregory, Scott; Donati, J. -F.; Hussain, G. (2014-02-01) - Journal article
      The magnetic fields of young stars set their coronal properties and control their spin evolution via the star-disc interaction and outflows. Using 14 magnetic maps of 10 classical T Tauri stars (CTTSs) we investigate their ...
    • CSI 2264 : Simultaneous optical and infrared light curves of young disk-bearing stars in NGC 2264 with CoRoT and Spitzer - Evidence for multiple origins of variability 

      Cody, A.M.; Stauffer, J.; Baglin, A.; Micela, G.; Rebull, L.M.; Flaccomio, E.; Morales-Calderón, M.; Aigrain, S.; Bouvier, J.; Hillenbrand, L.A.; Gutermuth, R.; Song, I.; Turner, N.; Alencar, S.H.P.; Zwintz, K.; Plavchan, P.; Carpenter, J.; Findeisen, K.; Carey, S.; Terebey, S.; Hartmann, L.; Calvet, N.; Teixeira, P.; Vrba, F.J.; Wolk, S.; Covey, K.; Poppenhaeger, K.; Günther, H.M.; Forbrich, J.; Whitney, B.; Affer, L.; Herbst, W.; Hora, J.; Barrado, D.; Holtzman, J.; Marchis, F.; Wood, K.; Guimarães, M.M.; Lillo Box, J.; Gillen, E.; McQuillan, A.; Espaillat, C.; Allen, L.; D'Alessio, P.; Favata, F. (2014-04-01) - Journal article
      We present the Coordinated Synoptic Investigation of NGC 2264, a continuous 30 day multi-wavelength photometric monitoring campaign on more than 1000 young cluster members using 16 telescopes. The unprecedented combination ...
    • Millimeter observations of the disk around GW Ori 

      Fang, M.; Sicilia-Aguilar, A.; Wilner, D.; Wang, Y.; Roccatagliata, V.; Fedele, D.; Wang, J. Z. (2017-07) - Journal article
      The GW Ori system is a pre-main sequence triple system (GW Ori A/B/C) with companions (GW Ori B/C) at ∼1 AU and ∼8 AU, respectively, from the primary (GW Ori A). The primary of the system has a mass of 3.9 M⊙, but shows a ...
    • Monte Carlo radiation transfer studies of protoplanetary environments 

      Walker, Christina H. (University of St Andrews, 2007-06-19) - Thesis
      Monte Carlo radiation transfer provides an efficient modelling tool for probing the dusty local environment of young stars. Within this thesis, such theoretical models are used to study the disk structure of objects across ...