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wyatt
https://people.ast.cam.ac.uk/~wyatt/wyatt_lyot07.pdf18 Jun 2007: Good news for TPF (look at oldstars). Bad news for explaining systemswith 25µm excess many of whichhave f>1000fmax and so must betransient. ... Late heavy bombardment model of (Gomes et al. 2005). 20. Conclusions 1 (Good news)Most disk radial structure -
Quasars and Galaxies at the Highest Redshifts
https://people.ast.cam.ac.uk/~rgm/presentations/20050922-Crafoord-Symposium.ppt8 Mar 2006: GOOD NEWS. The 1.0 to 1.8 micron IR sky is very dark between the OH lines which contain 95% of broad band background. ... THE NOT SO GOOD NEWS. The narrowest gaps are narrower than in the optical; filter widths of 0.1 per cent are needed compared with 1% -
Debris disk dynamical theory Mark Wyatt Institute of Astronomy, ...
https://people.ast.cam.ac.uk/~wyatt/MarkWyatt_Spitzer2008Conference.pdf12 Jan 2009: Sub-mm. Far-IR. Mid-IR. Good news: different wavelengths see different grain sizes and different structures. ... Bad news: both spatial distribution τ1/r and temperature of far-IR dust implies mass loss of 2M/Myr. -
Oxford Meeting
https://people.ast.cam.ac.uk/~rgm/presentations/20060412-SKA-Meeting_Oxford.ppt15 Apr 2006: Infrared OH Sky Observations: Mahaira etal, 1993, PASP. GOOD NEWS. The 1.0 to 1.8 micron IR sky is very dark between the OH lines which contain 95% of broad ... THE NOT SO GOOD NEWS. The narrowest gaps are narrower than in the optical; filter widths of
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