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23 Jul 2014: primordial protoplanetary disk (Watson et al.

21 Jan 2014: 4.8. Schneider et al. (2013)report a detection in the XMM-Newton Serendipitous Source Cat-alog (Watson et al.

22 Aug 2014: arX. iv:1. 408. 4116. v1 [. astr. o-ph. EP. ] 18. Aug. 201. 4Mon. Not. R. Astron. Soc.000, 000–000 (0000) Printed 20 August 2014 (MN LATEX style file v2.2). Do Two Temperature Debris Disks Have Multiple Belts? G. M. Kennedy, M. C. WyattInstitute

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.

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,

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