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13 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

21 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

23 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,.

17 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

2 Jul 2014: yielding the ratio of the total cross-sectional area on op-posing sides of the disc.

22 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;