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14 Nov 2013: How-ever, given that all three lie along a line of Fν λ. ... 2009).The suggestion that the entire HR 8799 system may be. coplanar is consistent with the results of Watson et al.(2011) and Greaves et al.

31 Jul 2018: This implies a very massive initial disc and efficientplanetesimal formation at large radii. ... parameters toour reference parametric model (3-power law surface densitywith a Gaussian gap).

4 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.

2 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.

15 Mar 2016: 2007), but could have a dramatic effect on the emission spectrum of theplanet. ... Typically the total mass of debris created in a giant impact iswell known.

7 Oct 2016: The origin of this hot dust is a matter of consid-erable debate. ... Nevertheless,a growing number of systems host planets and debris(Wyatt et al.

7 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.