Search

Search Funnelback University

Search powered by Funnelback
10 results 20 results 50 results
Relevance Date (Newest first) Date (Oldest first) Title (A-Z) Title (Z-A) Distance URL (A-Z) URL (Z-A) Shuffle
1 - 4 of 4 search results for `good news` |u:people.ast.cam.ac.uk

  1. Fully-matching results

  2. wyatt

    https://people.ast.cam.ac.uk/~wyatt/wyatt_lyot07.pdf
    18 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

  3. Quasars and Galaxies at the Highest Redshifts

    https://people.ast.cam.ac.uk/~rgm/presentations/20050922-Crafoord-Symposium.ppt
    8 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%

  4. Debris disk dynamical theory Mark Wyatt Institute of Astronomy, ...

    https://people.ast.cam.ac.uk/~wyatt/MarkWyatt_Spitzer2008Conference.pdf
    12 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.

  5. Oxford Meeting

    https://people.ast.cam.ac.uk/~rgm/presentations/20060412-SKA-Meeting_Oxford.ppt
    15 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

Refine your results

Date

Search history

Recently clicked results

Recently clicked results

Your click history is empty.

Recent searches

Recent searches

Your search history is empty.