Browsing by Author "Kamp, I."

Now showing items 1-5 of 5

    • Consistent dust and gas models for protoplanetary disks I. Disk shape, dust settling, opacities, and PAHs 
      Woitke, P.; Min, M.; Pinte, Christophe; Thi, W. F.; Kamp, I.; Rab, C.; Anthonioz, F.; Antonellini, S.; Baldovin Saavedra, C.; Carmona, A.; Dominik, C.; Dionatos, O.; Greaves, J.; Guedel, M.; Ilee, J. D.; Liebhart, A.; Menard, F.; Rigon, L.; Waters, L. B. F. M.; Aresu, G.; Meijerink, R.; Spaans, M. (EDP SCIENCES, 2016)
      We propose a set of standard assumptions for the modelling of Class II and III protoplanetary disks, which includes detailed continuum radiative transfer, thermo-chemical modelling of gas and ice, and line radiative transfer ...
    • Nature of the gas and dust around 51 Ophiuchi : Modelling continuum and Herschel line observations 
      Thi, W. F.; Ménard, Francois; Meeus, G.; Carmona, A.; Riviere Marichalar, P.; Augereau, J. C.; Kamp, I.; Woitke, P.; Pinte, Christophe; Mendigutía, I.; Eiroa, C.; Montesinos, B.; Britain, S.; Dent, W. (EDP Sciences, 2013)
      Context. Circumstellar disc evolution is paramount for the understanding of planet formation. The gas in protoplanetary discs large program (GASPS) aims at determining the circumstellar gas and solid mass around ∼250 ...
    • Probing protoplanetary disk evolution in the Chamaeleon II region 
      Villenave, M.; Ménard, F.; Dent, W. R. F.; Benisty, Myriam; Van der Plas, G.; Williams, J. P.; Ansdell, M.; Ribas, A.; Cáceres, C.; Cánovas, H.; Cieza, L.; Hales, A.; Kamp, I.; Pinte, C.; Principe, D. A.; Schreiber, M. R. (EDP Sciences, 2021)
      Context. Characterizing the evolution of protoplanetary disks is necessary to improve our understanding of planet formation. Constraints on both dust and gas are needed to determine the dominant disk dissipation ...
    • Radiation thermo-chemical models of protoplanetary discs IV. Modelling CO ro-vibrational emission from ... 
      Thi, W. F.; Kamp, I.; Woitke, P.; Van der Plas, Gerrit; Bertelsen, R.; Wiesenfeld, L. (EDP Sciences, 2013)
      Context. The carbon monoxide (CO) ro-vibrational emission from discs around Herbig Ae stars and T Tauri stars with strong ultraviolet emissions suggests that fluorescence pumping from the ground X1Σ+ to the electronic A1Π ...
    • Water vapor in the protoplanetary disk of DG Tau 
      Podio, L.; Kamp, I.; Codella, C.; Cabrit, S.; Nisini, B.; Dougados, C.; Sandell, G.; Williams, J. P.; Testi, L.; Thi, W. F.; Woitke, P.; Meijerink, R.; Spaans, M.; Aresu, G.; Ménard, Francois; Pinte, Christophe (The American Astronomical Society, 2013)
      Water is key in the evolution of protoplanetary disks and the formation of comets and icy/water planets. While high-excitation water lines originating in the hot inner disk have been detected in several T Tauri stars ...