Johan Olofsson MPIA Heidelberg

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The importance of the field-of-view ‣ The outer disk is in the Pionier, MIDI and SAM field-of-view ‣ Over-resolved, extended emission: drop in V 2 at short baselines ‣ Constraints on the outer disk, even with Pionier
A candidate companion ‣ Huélamo et al. (2011): NaCo/SAM closure phases w/ binary model ‣ L’-band detection, distance of 6.7 AU (in the gap), mass < 80 M Jup ‣ Closure phases: departure from centro-symmetry ‣ Anisotropic (forward) scattering: asymmetric surface brightness
Page 1 and 2: Planetary formation in transition a
Page 3 and 4: Giant & telluric planetary formatio
Page 5 and 6: The transition disk around TCha ‣
Page 7 and 8: The inner disk ‣ Narrow disk: 0.0
Page 9: The outer disk ‣ Most likely narr
Page 13 and 14: Hints for a companion ‣ Large gap
Page 16 and 17: Debris disk Final product of star f
Page 18 and 19: Warm debris disk around HD 113766 A
Page 20 and 21: One or two dust belts ‣ One dust
Page 22 and 23: Origin of the dust ‣ Massive coll
Page 24 and 25: Origin of the dust ‣ HD 113766 A:
Page 26: Take away messages ‣ SED modeling

Johan Olofsson MPIA Heidelberg

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