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27 Jul 2010: The outcome is summarisedin Fig. 6. 4.4.1 Radiation pressure. Radiation pressure is a radial force which acts in the op-posite direction to the star’s gravity.

8 Jul 2020: Finally, the detection of this gas is also a new op-portunity to study mechanisms that can transport angularmomentum in discs and may be beneficial for our under-standing of the ... We also compute CN masses in non-LTE assuming op-tically thin emission

17 Jan 2020: Evidence of misaligned inner discs has also beenrecently inferred for several systems using high-contrast op-tical/infrared images, which have revealed shadows in theouter disc cast by unseen inclined inner

14 Sep 2015: map reproduces the input op-tical depths very closely.

3 Nov 2008: arX. iv:0. 810. 5087. v1 [. astr. o-ph. ] 28. Oct. 200. 8Astronomy & Astrophysicsmanuscript no. 10706 c ESO 2008October 28, 2008. Resolved debris disk emission around η Tel: a young Solar Systemor ongoing planet formation? R. Smith1, L.J. Churcher1,

23 Aug 2018: 2017, Fig. A1, bottom). The high op-tical depth in the mid-plane would in fact shield the smallgrains from sublimation.

23 Sep 2016: before through modelling observations of op-tical and near-IR scattered light from the dust disk (e.g.Ahmic et al.

8 Nov 2011: It is interesting to note that the op-timum position for the inner planet is not as close to thestar as the outer planet could possibly scatter particles

19 Apr 2006: To probe the nature of the Vega disk further, wehave fitted it with models including realistic grain op-tical properties.

2 Nov 2015: Road, Cambridge, UK9 Department of Astronomy, Yale University, New Haven, CT10 Visiting Astronomer, NASA Infrared Telescope Facility, op-.