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The Triple Alpha Process for Helium Fusion Mathematics at ...
https://people.ast.cam.ac.uk/~cat/maths/maths.html21 Nov 2016: Tests. Applicants will be required to sit a one-hour non-calculator pre-interview test in mathematical skills during their interview visit. ... The tests will not be based on any particular syllabus and no past papers are available. -
MATHEMATICAL TRIPOS Part III Friday, 27 May, 2016 1:30 ...
https://people.ast.cam.ac.uk/~wyatt/psd_exam2016.pdf16 Sep 2016: 3. 2. Consider the motion of a test particle in the gravitational potential of a binarycomprised of two bodies of mass M1 and M2 M1. ... Part III, Paper 316 [TURN OVER. 4. 3. Consider the evolution of a test particle due to the secular perturbations of -
Mon. Not. R. Astron. Soc. 000, 1–8 (2016) Printed ...
https://people.ast.cam.ac.uk/~wyatt/ghmm16.pdf21 Jul 2016: 3.2 CO spectroscopy. Figure 3 shows the CO spectrum towards HD 32297, reduced bytwo different methods to test for robustness. ... 10 100. 1.0. 8. 6. 4. 2. 0. KS–Test Comparison Cumulative Fraction Plot. -
arX iv:1 601. 0686 6v1 [as tro- ph.E P] ...
https://people.ast.cam.ac.uk/~wyatt/dhmh16.pdf27 Jan 2016: the phase fluctuations but on-sky verification tests haveshown that large phase jumps can occasionally occur andcause fringe jumps (even with the phase loop running at1 kHz). -
arX iv:1 604. 0828 6v1 [ast ro-p h.E P] ...
https://people.ast.cam.ac.uk/~wyatt/mcbe16.pdf29 Apr 2016: 2014). To test this hypothesis we have mea-sured the degree of polarization of six hot dust stars with-out any notable excess at mid- or far-infrared wavelengthsusing the HIgh -
arX iv:1 610. 0071 4v1 [as tro- ph.E P] ...
https://people.ast.cam.ac.uk/~wyatt/wbjm16.pdf7 Oct 2016: 1987), showedhow the ultimate fate of any test particles encounteringand subsequently being scattered by a planet depends onthe planet’s mass and semimajor axis. ... 2.5 Applicability to scattered planets. The division of parameter space described in -
Mon. Not. R. Astron. Soc. 000, 1–16 (2002) Printed ...
https://people.ast.cam.ac.uk/~wyatt/kwcp16.pdf7 Jun 2016: To test thedependence on the IRF, we fix Ṁ/Ṁ0 = 1 and we createa second χ2 map, shown in Fig. -
MNRAS 000, 1–12 (2015) Preprint 12 May 2016 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mmsw16.pdf17 May 2016: To test the significance of this detec-tion and whether this could be a product of our image synthesismethod, we produce Clean images obtaining roughly the same re-sults. -
MNRAS 000, 1–21 (2016) Preprint 23 September 2016 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mdwk16.pdf23 Sep 2016: MNRAS 000, 1–21 (2016) Preprint 23 September 2016 Compiled using MNRAS LATEX style file v3.0. Exocometary gas structure, origin and physical propertiesaround β Pictoris through ALMA CO multi-transitionobservations. L. Matrà1,2?, W. R. F. Dent3, -
Space Science Reviews manuscript No.(will be inserted by the ...
https://people.ast.cam.ac.uk/~wyatt/wj16.pdf15 Mar 2016: Debris particles are massless test particles, and no accountis made for collisional erosion. -
MNRAS 000, 1–22 (2016) Preprint 7 November 2016 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mwpm16.pdf7 Nov 2016: In order to test the latter scenario andsee if the disc morphology can be explained by self-stirring,we considered a second model that consists of a parametricself-stirred disc based
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