Modelling planet-forming circumstellar discs - Herschel

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Gas in Proto<strong>planet</strong>ary Disks •First •Prev •Next •Last •Go Back •Full Screen •Close •Quit
PROto<strong>planet</strong>ary DIsk MOdel main paper → Woitke, Kamp & Thi (2009, A&A 501, 383) improved RT coupling → Kamp et al. (2010, A&A 510, 18) inner rim & SED calculation → Thi, Woitke & Kamp (2011, MNRAS 412, 711) PAH charge & line transfer → Woitke et al. (2011, A&A 534, 44) X-ray chemistry & heating → Aresu et al. (2011, A&A 526, 163) application to individual targets → 7 papers so far (2010 – 2012) this conference → used in 4 talks, 8 posters (!) •First •Prev •Next •Last •Go Back •Full Screen •Close •Quit
Page 1 and 2: Modelling Planet-forming Circumstel
Page 3: What means (radiation) thermo-chemi
Page 7 and 8: Heating & Cooling � Γk(Tgas, ni,
Page 9 and 10: κ [cm 2 /g(dust)] Disc dust is spe
Page 11 and 12: Radiation thermo-chemical disc mode
Page 13 and 14: Some remarkable results and latest
Page 15 and 16: z / r Dust and Gas Temperature L⋆
Page 17 and 18: Do the models agree? Bruderer et al
Page 19 and 20: Using optical - sub-mm lines to con
Page 21 and 22: Important results from Herschel •
Page 23 and 24: HD 100546: analysis of PACS/DIGIT d
Page 25 and 26: z [AU] 100 10 1 0.1 0.01 HD 169142:
Page 27 and 28: Herschel Water Lines I Riviere-Mari
Page 29 and 30: log ν F ν [erg/cm 2 /s] z [AU] -1
Page 31 and 32: Bad things (major uncertainties)

Modelling planet-forming circumstellar discs - Herschel

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