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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-. -
MNRAS 000, 1–21 (2022) Preprint 28September 2022 Compiled…
https://people.ast.cam.ac.uk/~wyatt/lwkk22.pdf29 Sep 2022: d 0.780 3.8890.004 71.50.7J f 1.24 3.0350.184 9516H f 1.65 2.5750.18 9816KS f 2.16 2.4230.242 7116. -
MNRAS 000, 1–12 (2021) Preprint 25February 2022 Compiled…
https://people.ast.cam.ac.uk/~wyatt/ckak22.pdf25 Feb 2022: DiscFlux (mJy) 1.840.220.21 1.830.210.21. Radius (au) 70.24.14.7 77.78.07.1 69.9. 0.90.8 107. ... GSC07396-00759’s disc’s radius of 70au is about double that ofAUMic’s disc’s radius of 24-40au (Daley et al. -
MNRAS 000, 1–?? (2017) Preprint 30 May 2022 Compiled ...
https://people.ast.cam.ac.uk/~bothwell/Files/MASCOT.pdf30 May 2022: ExploitingMulti Unit Spectroscopic Explorer (MUSE) observations at 50100pc scale resolution in 24 nearby star-forming galaxies, the authorsselected a sample of individual DIG/LI(N)ER - HII region pairs lo-cated -
MNRAS 000, 1–16 (2021) Preprint 9 February 2022 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/hwm22.pdf9 Feb 2022: 5smooth(A) = 46(A, 0, 6) 26(A, 10, 4) 6(A, 14, 10), (24).
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