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31 - 40 of 352 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 352 match some words.

  1. Results that match 1 of 2 words

  2. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_16.pdf
    10 Nov 2017: Evidence for kinematically distinct outflows – discrete mass-loss episodes (strongly asymmetric)• Expansion velocities 40-50km/s• Kinematic age estimates for features, from distance/velocity, are 200, 400 and 900 years• Smallest

  3. Astronomy & Astrophysics manuscript no. LIFE_paper_1_FINAL_EDITED …

    https://people.ast.cam.ac.uk/~wyatt/qofk22.pdf
    18 Apr 2022: 11 174718. 11910 123109310. 638406 245. Number of detectable planets. 0 200 400. ... Sub-Neptunes Sub-Jovians0. 50. 100. 150. 200. 250. 300. 350. Det. ecta.

  4. Chapter 2 - Operating the software

    https://people.ast.cam.ac.uk/~optics/cirsi/docs/pixcel/20010508/chapter2.htm
    16 Jun 2015: Base Electronics base pixel value, typically 200-1000 and is updated periodically.

  5. MNRAS 000, 1–6 (2016) Preprint 13 July 2016 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/agwk16.pdf
    13 Jul 2016: 0 100 200 300 400 500. UV Distance [kλ]. 100. 0. ... 100. 200. 300. Re(v. ) [m. Jy]. 0 100 200 300 400.

  6. LOCAL HEATING IN THE GALACTIC CENTER WESTERN ARC N. ...

    https://people.ast.cam.ac.uk/~wyatt/mtpf03.pdf
    19 Apr 2006: Dust emissionpeaks are resolved with source sizes of 200 to 500 (1.7 104 to4.3 104 AU).

  7. MGB thesis Chapter 3

    https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter3.htm
    16 Jun 2015: [Chapter 3: Camera. Outline. This chapter describes the near infrared camera built for COAST. It examines the properties required from the camera system, the range of devices available and the factors involved in the choice of detector. The design,

  8. Debris discs around nearby solar analogues

    https://people.ast.cam.ac.uk/~wyatt/gwb09.pdf
    8 Jul 2009: e. upto approximately 200 au radius for stars at 12–15 pc distance. ... For five precise (G2 V) solar analogues,the fitted disc radii are 100–200 au (Krivov et al.

  9. L141 The Astrophysical Journal, 532:L141–L144, 2000 April 1q 2000. ...

    https://people.ast.cam.ac.uk/~wyatt/ftpk00.pdf
    19 Apr 2006: Compared to the fullextent of the mid-IR–emitting size of the disk (200 AU), therelatively small values of the dust FWHM sizes suggest thatthe mid-IR emission is sharply peaked ... extends out to at least a radius of 100 (200 AU) fromthe star in the

  10. Searching for Saturn's Irregular Satellite Swarm with Spitzer

    https://people.ast.cam.ac.uk/~wyatt/kwss11.pdf
    29 Jun 2012: Stansberry. OFF ON IE IW. -600 -400 -200 0 200 400 600offset (Saturn radii). ... 400. -200. 0. 200. 400. offs. et (. Sat. urn. radi.

  11. PDF/48/aa5873-06.pdf.url

    https://people.ast.cam.ac.uk/~wyatt/lwbd06.pdf
    14 Dec 2006: 2004), we estimate for the firsttime the detection rate of cold debris disks around field M-dwarfs with ages between 20 and 200 Myr. ... al. 2005), the Castor moving group(200 Myr), the Ursa Maj moving group (500 100 Myr asrevised by King et al.

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