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A planet-forming circumbinary disc in a polar configura-tion Grant ...
https://people.ast.cam.ac.uk/~wyatt/kmfm19.pdf17 Jan 2019: 4605. 0.046. 200.0. 4635. F. F = 0.0468.6e 058.7e 05. 0.054. ... a = 1.200.030.03. 0.495. 0.510. 0.525. 0.540. e. e = 0.520.010.01. -
Extrasolar Kuiper Belts Mark C. Wyatt Abstract Extrasolar debris ...
https://people.ast.cam.ac.uk/~wyatt/wyat19.pdf26 Sep 2019: Onepossibility is that these form directly from the protoplanetary disk (rather than fromthe collisional growth of smaller planetesimals), or it could be that a massive diskof 200 km planetesimals can stir -
MNRAS 000, 1–21 (2018) Preprint 11 July 2019 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/yksw19.pdf11 Jul 2019: We choose to focus only on excesses at70 and 100 µm, corresponding to typical dust tempera-tures of order 30–200 K. ... HD 165908 2.9 45 4 1.6E-05 9.2E-07 64 11 241 40HD 172555 8.0 200 1 3.8E-04 2.7E-06 5.5 0.1 -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture15.pdf19 Nov 2019: Typical values rangefrom v ' 200 km s1 in A-type supergiants to v ' 3000 km s1 inearly O-type stars.
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