Search

23 Nov 2021: These instru-ments reveal a wealth of substructures within disks, forboth targeted (e.g. ... We assumehere a gas-to-dust mass ratio of 100 and indicate the.

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).

18 Aug 2020: We start with a simple estimate. Assuming the PPDmass to be 0.1M? ... A-stars with2 solar masses) can be higher by a factor 2.7.

29 Apr 2008: 2005), thoughtto be there because this is a young (12Myr, Zuckerman et al. ... We con-sider a detection to be whereS op > 3. 4.1.1.

10 Feb 2021: 2017), a possibility also not ruled out by far-IRsurveys of star forming regions. ... Withinthe inner 0.68′′ radius circle there is a 2.8𝜎 significant detection.

28 Oct 2013: Kervella P., Thévenin F., Di Folco E., Ségransan D., 2004,A&A 426, 297. ... von Braun K. et al., 2011, ApJ 729, L26. Watson C.A.

17 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.

22 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.

29 Apr 2016: arX. iv:1. 604. 0828. 6v1. [ast. ro-p. h.E. P]. 28 A. ... by high orbital eccentricity comets,is likewise difficult to achieve from a dynamical perspective.

2 Nov 2015: M. Ansdell1,10, E. Gaidos2,3,4,10, S. A. Rappaport5, T. L. Jacobs6, D. ... M. LaCourse6, K. J. Jek6, A. W. Mann7,10, M.C. Wyatt8, G.