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1 - 10 of 14 search results for :pc53 24 / |u:people.ast.cam.ac.uk where 0 match all words and 14 match some words.

  1. Results that match 1 of 2 words

  2. Peer-reviewed Publications See here for latest list of…

    https://people.ast.cam.ac.uk/~nmadhu/Nikku_Madhusudhan/Publications.html
    27 Aug 2022: 24. A. M. S. Smith, D. R. Anderson, N. Madhusudhan, SuperWasp Team, et al. ... 2009, ApJ, 707, 24 . 5. N. Madhusudhan & J. Winn, Empirical Constraints on Trojan Companions and Orbital Eccentricities in 25.

  3. Robin Catchpole

    https://people.ast.cam.ac.uk/~catchpol/
    13 Dec 2022: and spent the next 24 years, working first at the Radcliffe Observatory in Pretoria and then at the SAAO in Cape Town.

  4. DRAFT VERSION MAY 24, 2022Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/hcrs22.pdf
    24 May 2022: 18. Michael C. Liu ,19 Mickael Bonnefoy,20 Thayne Currie,21 Michael McElwain ,22 Stanimir Metchev,23 Mark Wyatt,24 Olivier Absil ,25. ... Sebastian Marino,45, 24 Mark Marley,46 Raquel Martinez ,47 Christian Marois ,48, 49 Brenda Matthews ,48, 49

  5. Nikku Madhusudhan

    https://people.ast.cam.ac.uk/~nmadhu/Nikku_Madhusudhan/Home.html
    27 Aug 2022: Madhusudhan & Seager, 2009, The Astrophysical Journal, 707, 24. The so-called “Million Model Approach” to atmospheric modeling of exoplanets.

  6. M. Pettini: Structure and Evolution of Stars — Lecture ...

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture14.pdf
    20 Nov 2022: 14.24), so that the total kinetic energyis EK = CM. 5/3/R2, where C is a constant. ... ne =M. µmp. (4πR3. 3. )1(14.31). which, when combined with (14.24), gives:.

  7. Research

    https://people.ast.cam.ac.uk/~nmadhu/Nikku_Madhusudhan/Research.html
    27 Aug 2022: First statistical retrieval method for exoplanetary atmospheres (Madhusudhan & Seager, 2009, ApJ, 707, 24). •

  8. M. Pettini: Structure and Evolution of Stars — Lecture ...

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture08.pdf
    30 Oct 2022: The star would collapse on a free-fall timescalegiven by:. tff =. 2R. g(8.24). where R is the star radius (recall r = 12at2 for a body experiencing accel-.

  9. DRAFT VERSION OCTOBER 25, 2022Typeset using LATEX default style ...

    https://people.ast.cam.ac.uk/~wyatt/hmsu22.pdf
    25 Oct 2022: 8010. 0. r o. ut. [au. ]. 0.06. 0.12. 0.18. 0.24. ... rout [au]. 0.06. 0.12. 0.18. 0.24. 0.30. h. 70 75 80 85.

  10. Astronomy & Astrophysics manuscript no. paperKBA_Av2subarxiv ©ESO …

    https://people.ast.cam.ac.uk/~wyatt/kpgm21.pdf
    14 Feb 2022: Brown, G.N.; Ziegler, W.T., 1979, J. Chem. Eng. Data, 24, 319-30Cordiner M. ... The volatiles with subli-mation temperatures lower than 40 K are N2 (22 K), O2 (24 K),CO (25 K), and CH4 (31 K) with the sublimation temperaturegiven in parenthesis (Yamamoto

  11. M. Pettini: Structure and Evolution of Stars — Lecture ...

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture06.pdf
    17 Oct 2022: 24/06/2011 16:38Curves of growth: metallicity and vt. Page 1 of 1http://www.lna.br/albert/preprints/preprint04_00/node7.html. ... 06 52 Te 2.18 0.0310 Ne [7.93 0.10] 1.12 53 I 1.55 0.0811 Na 6.24 0.04 6.27 0.02 54 Xe

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