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Robin Catchpole
https://people.ast.cam.ac.uk/~catchpol/13 Dec 2022: It was described in the British Sundial Society Bulletin, vol.20,June 2008. -
Peer-reviewed Publications See here for latest list of…
https://people.ast.cam.ac.uk/~nmadhu/Nikku_Madhusudhan/Publications.html27 Aug 2022: Thermal Inversions, Spectra, and Formation conditions, 2011, ApJ, 743, 191. 20. -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture08.pdf30 Oct 2022: 8.20). where: (i) Mr is the mass enclosed within radius r; (ii) A is the area ofthe base of the cylinder; and (iii) dP is the difference in pressure (definedas ... VIII. Fig. 1. Stream lines of meridional circulation in a rotating 20 M! -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture06.pdf17 Oct 2022: Application of the line-depth ratio method can yield very high temper-ature resolution, as high as a few K, which is 10–20 times better thanthe accuracy with which the ... The solid line is deemed to fit best. The spectrum usedfor this abundance -
MNRAS 000, 1–12 (2021) Preprint 25February 2022 Compiled…
https://people.ast.cam.ac.uk/~wyatt/ckak22.pdf25 Feb 2022: MNRAS 000, 1–12 (2021). 10 P. F. Cronin-Coltsmann et al. 20 15 10 5 0 5 10 15 20VelocityBary (km/s). ... 2015105. 0. 5. 10. 15. 20. Flux. (mJy. /cha. nnel. ). Spatial Filter. Spectro-spatial Filter NW Towards us. Spectro-spatial Filter SE Towards us. -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture14.pdf20 Nov 2022: 24π2h̄3. (6π2h̄3ρegme. )4/3 K2ρ4/3e (14.20). with. K2 =πh̄c. 4m4/3e. (6. gπ. ... 1/3. What eqs. 14.18 and 14.20 show us is a result that has been stated before:in degenerate gas, the pressure depends only on density and is independentof -
DRAFT VERSION OCTOBER 25, 2022Typeset using LATEX default style ...
https://people.ast.cam.ac.uk/~wyatt/hmsu22.pdf25 Oct 2022: 85. i[. ]. 30 60 90 120. rin [au]. 20 40 60 80 100. ... log10MCO (M )1.6. 51.8. 01.9. 52.1. 0. M (M )8 12 16 20 24. -
Astronomy & Astrophysics manuscript no. LIFE_paper_1_FINAL_EDITED …
https://people.ast.cam.ac.uk/~wyatt/qofk22.pdf18 Apr 2022: Ehrenreich16,S. Ertel17, 18 M. Fridlund19, 20, A. García Muñoz11, C. Gascón21, J. ... 2021). Somemajor detections were even made within 20 pc of the Sun with. -
Astronomy & Astrophysics manuscript no. paperKBA_Av2subarxiv ©ESO …
https://people.ast.cam.ac.uk/~wyatt/kpgm21.pdf14 Feb 2022: total CO massof 2 1012 M (i.e., 20 times the CO quantity that was lost. ... 2019); (19): Läuteret al. (2020); (20): Womack et al. (2017); (21): Lellouch et al.(2017); (22): Rauer et al. -
MNRAS 000, 1–21 (2022) Preprint 28September 2022 Compiled…
https://people.ast.cam.ac.uk/~wyatt/lwkk22.pdf29 Sep 2022: 01443.T,PI:Lovell).Eachschedul-ingblockobserved for 49minutes on source, andwere conductedon the4-Dec2019, 20-Dec2019, and2x21-Dec2019. ... 131 61.1 151 193 0.07 -0.20 - - 98(0.0028) (9) (3.8) (5) (13) (0.04) (0.07) - - (19).
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