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Five steps in the evolution from protoplanetary to debrisdisk ...
https://people.ast.cam.ac.uk/~wyatt/wpkm15.pdf17 Dec 2014: Thus the dividingline is usually placed at f 0.01, which is around thelevel at which the dust might be expected to become op-tically thin in the radial direction to -
Mon. Not. R. Astron. Soc. 000, 1–22 (2002) Printed ...
https://people.ast.cam.ac.uk/~wyatt/pw14.pdf2 Jul 2014: yielding the ratio of the total cross-sectional area on op-posing sides of the disc. -
arX iv:1 408. 4116 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/kw14.pdf22 Aug 2014: For all systems, photometry ranging from op-tical to sub-mm wavelengths is compiled from a wide vari-ety of sources, including all-sky surveys such as Hipparcos(Perryman & ESA 1997; -
arX iv:1 312. 4531 v2 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/kmlm13.pdf21 Jan 2014: However, this similarityrequires that both components are radially optically thickand op-tically thin in the viewing direction, or the opening anglesmust belarger. ... The length of this period is uncertain due to the possibilityof non-axisymmetry and an -
Irwin06draft.dvi
https://people.ast.cam.ac.uk/~wfcam/ukreview/Irwin06draft.pdf23 Jul 2014: Mon. Not. R. Astron. Soc. 000, 1–26 (2006) Printed 15 May 2013 (MN LATEX style file v2.2). Pipeline processing of wide-field near-infrared data fromWFCAM (draft - not for circulation). Mike Irwin1, Jim Lewis1, Marco Riello1, Simon Hodgkin1,. -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture05.pdf13 Oct 2014: The full calculation of stellar opacities is a major endeavour. For this rea-son, the Opacity Project (op) was set-up in 1984 as an international collab-oration to calculate the ... Similar work conducted at the LawrenceLivermore National Laboratory, the
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