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1 - 10 of 14 search results for TALK:PC53 20 |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. 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.

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

    https://people.ast.cam.ac.uk/~nmadhu/Nikku_Madhusudhan/Publications.html
    27 Aug 2022: Thermal Inversions, Spectra, and Formation conditions, 2011, ApJ, 743, 191. 20.

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

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture08.pdf
    30 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!

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

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture06.pdf
    17 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

  6. MNRAS 000, 1–12 (2021) Preprint 25February 2022 Compiled…

    https://people.ast.cam.ac.uk/~wyatt/ckak22.pdf
    25 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.

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

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture14.pdf
    20 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

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

    https://people.ast.cam.ac.uk/~wyatt/hmsu22.pdf
    25 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.

  9. Astronomy & Astrophysics manuscript no. LIFE_paper_1_FINAL_EDITED …

    https://people.ast.cam.ac.uk/~wyatt/qofk22.pdf
    18 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.

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

    https://people.ast.cam.ac.uk/~wyatt/kpgm21.pdf
    14 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.

  11. MNRAS 000, 1–21 (2022) Preprint 28September 2022 Compiled…

    https://people.ast.cam.ac.uk/~wyatt/lwkk22.pdf
    29 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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