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search results for `Watson A A` |u:people.ast.cam.ac.uk
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arX iv:1 312. 4531 v2 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/kmlm13.pdf21 Jan 2014: a useful evolutionary sequence it is important to interpret in-dividual objects carefully. ... 4.8. Schneider et al. (2013)report a detection in the XMM-Newton Serendipitous Source Cat-alog (Watson et al. -
Five steps in the evolution from protoplanetary to debrisdisk ...
https://people.ast.cam.ac.uk/~wyatt/wpkm15.pdf17 Dec 2014: mass component of a protoplanetary disk, is no longer. present in debris disks. ... this denomination. A catalogue summarising this class. is given in Thé et al. -
arX iv:1 408. 4116 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/kw14.pdf22 Aug 2014: Infra-red excess detections are generally well approxi-mated by a single blackbody. ... For example,ζ Lep shows evidence for extra emissionabove a blackbody around 10µm (Fig. -
TLA_large
https://people.ast.cam.ac.uk/~wyatt/tgmk14.pdf4 Dec 2014: Key words: surveys – binaries: general – circumstellar matter – stars: individual: A-stars –infrared: stars. ... Mi. HD. 8769. 6A. 7V28. 24. 450. UM. a(3. ,4). 22.0. -
arX iv:1 403. 6186 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/mmek14.pdf2 Jul 2014: J.P. Marshall, A. Moro-Martı́n, et al.: Herschel observations of exoplanet host stars. ... plored for a broad range of ages by e.g. Decin et al. -
Observations, Modeling and Theory of Debris Disks Brenda C. ...
https://people.ast.cam.ac.uk/~wyatt/mkwb14.pdf7 Jan 2014: stars are statistically indistinguishable,a result supported by DUNES data (Eiroa et al. ... Even in a transport-dominated disk, the largest planetes-imals are dominated by collisions.
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