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Nikku Madhusudhan
https://people.ast.cam.ac.uk/~nmadhu/Nikku_Madhusudhan/Home.html27 Aug 2022: Madhusudhan & Seager, 2009, The Astrophysical Journal, 707, 24. The so-called “Million Model Approach” to atmospheric modeling of exoplanets. -
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. -
Peer-reviewed Publications See here for latest list of…
https://people.ast.cam.ac.uk/~nmadhu/Nikku_Madhusudhan/Publications.html27 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. -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture14.pdf20 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:. -
Research
https://people.ast.cam.ac.uk/~nmadhu/Nikku_Madhusudhan/Research.html27 Aug 2022: First statistical retrieval method for exoplanetary atmospheres (Madhusudhan & Seager, 2009, ApJ, 707, 24). • -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture08.pdf30 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-. -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture06.pdf17 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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