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arX iv:1 201. 1911 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/kwsd12.pdf12 Jan 2012: 20. DE. C o. ffset. ("). -0.10. 0.04. 0.18. 0.32. 0.46. ... 0. 10. 20. DE. C o. ffset. ("). -0.08. 0.00. 0.08. -
Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...
https://people.ast.cam.ac.uk/~wyatt/bksm12.pdf5 Oct 2012: These 9 stars constitute the full sample of resolvedA star discs between 20 and 40 pc. ... PSF fit500 20.30.4 0.210.00 20.00.4 PSF fit. -
Draft version December 10, 2012Preprint typeset using LATEX style ...
https://people.ast.cam.ac.uk/~wyatt/bmkb12.pdf10 Dec 2012: 2000)V magnitude 4.25 Balona et al. (1994)Distance (pc) 20.46 0.15 Phillips et al. ... 6 Broekhoven-Fiene et al. 0 5 10 15 20 25Semimajor axis (arcsec). -
cv.dvi
https://people.ast.cam.ac.uk/~gpe/cv.pdf24 Jan 2012: J. Supp., 107, 20 1. [R97] Power Spectrum Analysis of the Stromlo-APM Redshift Survey. ... 20 authors, 2000, Astro. Lett. and Communications, 37, 161. [R138] Simulations of Deep Pencil-Beam Redshift Surveys N. -
mnr_21298_LR
https://people.ast.cam.ac.uk/~wyatt/wksm12.pdf7 Nov 2012: correction for a 20 arcsec aperture quoted by the PACS team2 of 17,20 and 26 per cent. ... sensitiv-ity for an extended source at 3.7 arcsec radius of 20.0 mag arcsec2. -
arX iv:1 211. 4898 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/lmsk12.pdf24 Nov 2012: This data filtering results in the sourceflux density being underestimated by 20 5% as discussedin detail by Kennedy et al. ... 100µm 0.99 408 2.2 1.2 312214 55 (100) 2 α 0 3.50.51 60 110 20. -
Dynamical effects of stellar massloss on a Kuiperlike belt
https://people.ast.cam.ac.uk/~wyatt/bmw11.pdf22 May 2012: Of the values of initialeccentricity and inclination tested here, the numerical simulationwith emax = 0.2 and imax = 20 scatters the most test particles.This implies that an analytic formulation for the ... A further numerical simulation with emax = 0.2 -
arX iv:1 205. 0004 v2 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/fgwg12.pdf9 Oct 2012: 4 Ju. n 20. 12Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 15 June 2012 (MN LATEX style file v2.2). -
1 A SELF-CONSISTENT MODEL OF THE CIRCUMSTELLAR DEBRIS CREATED ...
https://people.ast.cam.ac.uk/~wyatt/jlcm12.pdf23 Oct 2012: μm is attributed to the Si-O bond vibration of amorphous silica and, along with a secondary 20. ... 20. described at the beginning of this section. Although, the submicron obsidian grains with. -
mnr_20522_LR
https://people.ast.cam.ac.uk/~wyatt/vw12.pdf30 Oct 2012: Fig. 2 indicates that this bifurcation value is a factor of2–20 times as high as the Solar system’s post-main-sequence escapeboundary.
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