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12 Jan 2012: arX. iv:1. 201. 1911. v1 [. astr. o-ph. EP. ] 9. Jan. 2012. Mon. Not. R. Astron. Soc.000, 000–000 (0000) Printed 11 January 2012 (MN LATEX style file v2.2). 99 Herculis: Host to a Circumbinary Polar-ring Debris Disk. G. M. Kennedy1, M. C. Wyatt1,

23 Oct 2012: IRAS (1983) to WISE (2010). Our new spectral modeling work and calculations of the radiation. ... 3.2 – Particle Size Distributions. New spectral modeling work, using the same dust composition found in Li2009 and the same.

1 Aug 2012: New for this work was theadditional requirement of including a separate population oflarge cool grains with a > 100 μm. ... preferentially vaporizing the small end of an initial dust pop-ulation, leaving behind a remnant large dust population and

5 Oct 2012: Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 3 October 2012 (MN LATEX style file v2.2). Resolved Debris Discs Around A Stars in the HerschelDEBRIS Survey? Mark Booth1,2†, Grant Kennedy3, Bruce Sibthorpe4, Brenda C. Matthews2,1,Mark C.

24 Feb 2012: In prep. ABSTRACT. We present new MIDI interferometric and VISIR spectroscopic observations ofHD113766 and HD172555.

7 Jul 2012: 2009; Bryden et al. 2009;Dodson-Robinson et al. 2011). However, there is new tentative ev-idence that nearby stars with low-mass planetary systems are morelikely to harbour debris than

24 Nov 2012: of Physics, University of New South Wales, Sydney 2052, Australia15 Departamento de Astronoma, Universidad de Chile, Casilla 36-D, Santiago, Chile16 Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, ... We re-reduced the

7 Nov 2012: Physics, University of New South Wales, Sydney 2052, Australia15Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA.

19 Jun 2012: The semi-major axis, eccentricity and inclinationof the new orbits of the debris (a′, e′, I′) will be given by:.

23 Feb 2012: Itis important to note, however, that while our spectral modelingtechniques can provide important new information, they are alsocomplex. ... A number of new mineralspecies were studied and compared to the η Corvi spectrum,in an attempt to match the

19 Jan 2012: pronounced atλ 70µm.Here we present new simulations that show that this connection is qualitatively robust to a range of parameters: the massdistributionof the giant planets, the width and mass distribution