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41 - 50 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. 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

  3. 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.

  4. 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.

  5. arX iv:a stro -ph/ 0504 086 v1 4 A ...

    https://people.ast.cam.ac.uk/~wyatt/srms05.pdf
    19 Apr 2006: higher surface brightness at r >200 AU compared to the r4 power law. ... but has slightlyhigher surface brightness at r > 200 AU compared to ther4 power law.

  6. MNRAS 000, 1–17 (2023) Preprint 25 October 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/ckkl23.pdf
    22 Mar 2024: 200. 0. 200. 400. µJy. /Bea. m. Figure 1. Naturally weighted ALMA 880𝜇m images of our BPMG M-dwarf sample. ... 0. 200. 400. µJy. /Bea. m. Figure 2. Naturally weighted ALMA 880𝜇m image of TYC 7443-1102-1.The stellar location is marked with a.

  7. Mon. Not. R. Astron. Soc. 000, 1–8 (2016) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/ghmm16.pdf
    21 Jul 2016: A 200 km/svelocity range is shown around the stellar velocity in the heliocen-tric frame of 23.0 0.3 km/s (Torres et al. ... The wide-fit baseline yields a 10.5 sigma detection of 200.0 19.1 mK km/s.

  8. MNRAS 000, 1–14 (2020) Preprint 8October 2020 Compiled…

    https://people.ast.cam.ac.uk/~wyatt/xkwy20.pdf
    8 Oct 2020: 2015).Assuming thepriors stated above,we ran LOFTI on the relative Gaia measurements until 200,000orbits were accepted, and plot the joint posterior distributions inFig. ... 160. 200. 240. []. 10 15 20. m [MJup]. m [MJup] = 1422.

  9. https://people.ast.cam.ac.uk/~rgm/wfcsur/jsc_ridos.txt

    https://people.ast.cam.ac.uk/~rgm/wfcsur/jsc_ridos.txt
    1 Mar 1998: Hence in total the project life-span would be 4 years, with a survey area of 100-200 square degrees in up to seven colour bands. ... Hence in total the project life-span would be 4 years, with a survey area of 100-200 square degrees in up to seven

  10. Hard XMM sources

    https://people.ast.cam.ac.uk/~xmmssc/internal/xsrc_select/xsrc_hr3-err_gt0.html
    27 Mar 2002: 0.853.08. A 1837. 200. 2001-02-22. Y. -1.7. -1.8. 20.7. 0. 22.6. ... 0.210.31. A 1837. 200. 2001-02-22. Y. -1.4. 1.4. 15.5. -1. 17.4.

  11. Graphics produced by IDL

    https://people.ast.cam.ac.uk/~vasily/sdss/orphan/orphan6.pdf
    10 Apr 2009: 2. 3. 4. log(. g). 4.0 3.9 3.8 3.7 3.6log(Teff). 300 200 100 0 100 200 300Radial velocity (Galactic frame). ... 0. 20. 40. 60. Dec. 250 200 150 100RA. Orphan Stream: 17 < g < 19 => 20 < BHB distance (kpc) < 50.

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