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  1. Results that match 1 of 2 words

  2. 842 Publications of the Astronomical Society of the Pacific, ...

    https://people.ast.cam.ac.uk/~wyatt/mghw07.pdf
    18 Sep 2007: Basedon these analyses, Rhee et al. revised the fraction of nearby Astars with detected 60mm excess to 20%. ... typesystems) and young Sun-like stars (20 among 200 of the Gand K stars).
  3. MASS AND TEMPERATURE OF THE TWA 7 DEBRIS DISK ...

    https://people.ast.cam.ac.uk/~wyatt/mkw07.pdf
    3 Jul 2007: The absolute fluxcalibration is accurate to 20%–30%. Pointing was checked onthe source 1034293. ... HD 92945. K1 22 20–150 271 70 >0.002 40 Chen et al.
  4. arX iv:0 704. 3369 v1 [ astr o-ph ] ...

    https://people.ast.cam.ac.uk/~wyatt/mlpw07.pdf
    26 Apr 2007: The dashed lineis for a path in a disc with Rt = 20 AU. ... The disc is initially trun-cated at Rt = 20 AU unless otherwise stated.
  5. Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/wcg07.pdf
    18 Jul 2007: While ALMA can detect the brightest knownclass II disks out to 20 kpc, we are not aware of any young(< 10 Myr) cluster within the Milky Way which has a ... For example, extrapo-lation of the exoplanet semi-major axis distribution to 20 AUsuggests that
  6. Submitted to ApJ, 3 January 2007, accepted 22 March ...

    https://people.ast.cam.ac.uk/~wyatt/wssr07.pdf
    23 Mar 2007: Mmax =. (. 3.8 106ρr3.5(dr/r)DcM 0.5? tage. ). (. (12q 20)[1 1.25(e/I)2]0.5(18 9q)G(q, Xc). ). , ... 1-5 (diamond=small excess),. 5-20 (square=medium excess), > 20 (triangle=large excess).
  7. Microsoft PowerPoint - wyattpub

    https://people.ast.cam.ac.uk/~wyatt/wyatt_kobe06.pdf
    24 Apr 2007: 20 have planets• 18 have debris detected with IRAS• 1 has both• stars with planets are metal-rich (Fischer & Valenti 2005). • ... http://www.ast.cam.ac.uk/wyatt. 20. The planetesimal belt. Consider planetesimals orbiting the star at a distance r
  8. wyatt

    https://people.ast.cam.ac.uk/~wyatt/wyatt_lyot07.pdf
    18 Jun 2007: Late heavy bombardment model of (Gomes et al. 2005). 20. Conclusions 1 (Good news)Most disk radial structure explained by steady-state evolution of aplanetesimal belt due to collisions and radiation
  9. Archive: Chemical Informatics Letters

    https://www-jmg.ch.cam.ac.uk/CIL/archive/vol13.html
    5 Jan 2007: Chemical Informatics Letters. Editor:Volume 13. (1). Definition and exchange of crystallographic data. International Tables for Crystallography: Volume G: Definition and exchange of crystallographic data, edited by Sydney Hall and Brian McMahon, is
  10. Archive: Chemical Informatics Letters

    https://www-jmg.ch.cam.ac.uk/CIL/archive/vol14.html
    3 Jul 2007: Chemical Informatics Letters. Editor:Volume 14. (1). Computational Crystallography Toolbox. The Computational Crystallography Toolbox is an open source component of the PHENIX (Python-based Hierarchical ENvironment for Integrated Xtallography)
  11. Archive: Chemical Informatics Letters

    https://www-jmg.ch.cam.ac.uk/CIL/archive/vol15.html
    24 Aug 2007: Chemical Informatics Letters. Editor:Volume 15. (1). Optical Structure Recognition Application (OSRA). OSRA is a free program which converts pictures of molecules (in most common formats, including PDF, GIF, JPEG, PNG, TIFF) into SMILES. It can be

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