Search

14 Nov 2013: 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.

17 Dec 2014: Five steps in the evolution from protoplanetary to debrisdisk. M. C. Wyatt • O. Panić • G. M. Kennedy •. L. Matrà. Abstract The protoplanetary disks seen around Her-big Ae stars eventually dissipate leaving just a tenuousdebris disk,

4 Dec 2014: MNRAS 445, 2558–2573 (2014) doi:10.1093/mnras/stu1864. An unbiased study of debris discs around A-type stars with Herschel. N. D. Thureau,1‹ J. S. Greaves,1 B. C. Matthews,2,3 G. Kennedy,4 N. Phillips,5. M. Booth,2,3,6 G. Duchêne,7,8 J.

29 Apr 2016: arX. iv:1. 604. 0828. 6v1. [ast. ro-p. h.E. P]. 28 A. pr 2. 016. DRAF T VERS IONA P RIL 29, 2016Preprint typeset using LATEX style emulateapj v. 5/2/11. POLARIZATION MEASUREMENTS OF HOT DUST STARSAND THE LOCAL INTERSTELLAR MEDIUM. J. P. MARSHALL 1,2,

2 Nov 2015: Accepted to ApJ: October 28, 2015Preprint typeset using LATEX style emulateapj v. 5/2/11. YOUNG “DIPPER” STARS IN UPPER SCO AND ρ OPH OBSERVED BY K2. M. Ansdell1,10, E. Gaidos2,3,4,10, S. A. Rappaport5, T. L. Jacobs6, D. M. LaCourse6, K. J. Jek6

23 Dec 2017: WATSON,130 R.C. WEIR,4. KLAUS WENZEL,131 MICHAEL W. WILLIAMSON,56 JASON T. WRIGHT,10, 11, 132 M.

15 Mar 2016: Space Science Reviews manuscript No.(will be inserted by the editor). Insights into planet formation from debris disks. II. Giant impacts in extrasolar planetary systems. Mark C. Wyatt Alan P. Jackson. Received: date / Accepted: date. Abstract Giant

19 Feb 2018: MNRAS 475, 3046–3064 (2018) doi:10.1093/mnras/stx3188Advance Access publication 2017 December 11. Analysis of the Herschel DEBRIS Sun-like star sample. B. Sibthorpe,1,2‹ G. M. Kennedy,3 M. C. Wyatt,4 J.-F. Lestrade,5 J. S. Greaves,6. B. C.

31 Jul 2018: MNRAS 000, 1–19 (2015) Preprint 4 July 2018 Compiled using MNRAS LATEX style file v3.0. A gap in the planetesimal disc around HD 107146 andasymmetric warm dust emission revealed by ALMA. S. Marino,1?, J. Carpenter,2 M. C. Wyatt1, M. Booth3, S.

25 Nov 2015: arX. iv:1. 511. 0591. 9v1. [ast. ro-p. h.E. P]. 18 N. ov 2. 015. Mon. Not. R. Astron. Soc.000, 1–18 (2002) Printed 19 November 2015 (MN LATEX style file v2.2). IR-excesses around nearby Lambda Boo stars are caused by debrisdisks rather than ISM

29 Oct 2013: Le Bouquin et al. 2009; Watson et al.2011; Kennedy et al.

5 May 2017: arX. iv:1. 701. 0656. 8v1. [as. tro-. ph.S. R]. 23. Jan. 2017. rsos.royalsocietypublishing.org. Research. Article submitted to journal. Subject Areas:. astrophysics, extrasolar planets, stars. Keywords:. variable stars, protoplanetary disks,. debris

2 Jul 2014: arX. iv:1. 403. 6186. v1 [. astr. o-ph. EP. ] 24. Mar. 201. 4Astronomy & Astrophysicsmanuscript no. dunes˙debris˙exoplanets˙v18 c ESO 2014March 26, 2014. Correlations between the stellar, planetary and debris componentsof exoplanet systems

7 Jan 2014: Observations, Modeling and Theory of Debris Disks. Brenda C. MatthewsNational Research Council of Canada – Herzberg Astronomy & Astrophysics. Alexander V. KrivovFriedrich-Schiller-Universität Jena. Mark C. WyattUniversity of Cambridge. Geoffrey

7 Oct 2016: arX. iv:1. 610. 0071. 4v1. [as. tro-. ph.E. P] 3. Oct. 201. 6. MNRAS 000, 1–25 (2016) Preprint 5 October 2016 Compiled using MNRAS LATEX style file v3.0. How to design a planetary system for different scattering. outcomes: giant impact sweet spot,

16 Jun 2015: Spot a 00:47:33.410 -25:17:13.6 Spot i 00:47:33.013 -25:17:18.12 Spot n 00:47:33.063 -25:17:17.20

5 Jun 2007: Venemans(Cam),F. Walter(MPIA), N. Walton(Cam), S. Warren(IC), M. Watson(Leic), N. Webb(Toulouse),C. Wolf(Oxf), H.

5 Jul 2011: Mon. Not. R. Astron. Soc. 000, 1–20 (2010) Printed July 5, 2011 (MN LATEX style file v2.2). Multi-Wavelength Modelling of the β Leo Debris Disc: 1, 2 or 3planetesimal populations? L J Churcher 1†, M.C. Wyatt1, G. Duchêne2,3, B. Sibthorpe4, G.

28 Sep 2009: MJI is in communication with Watson Varricatt regarding the low light level non-linearity tests and also a revisit of the normal non-linearity tests. ... Watson and MJI will also be comparing dome flats with twilight sky flats.

5 Jun 2007: Venemans(Cam),F. Walter(MPIA), N. Walton(Cam), S. Warren(IC), M. Watson(Leic), N. Webb(Toulouse),C. Wolf(Oxf), H.