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1 - 6 of 6 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 6 match some words.

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

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture01.pdf
    19 Sep 2023: Most stars end their. Figure 1.7: Hubble Space Telescope image of the Helix Nebula, the prototypical andclosest planetary nebula, at a distance of only 200 pc.

  3. MNRAS 000, 1–16 (2022) Preprint 6 July 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/bwmd23.pdf
    11 Jul 2023: Rrk = Σirki=ick. ni4(Dk Di). 2 πvrelV. , (11). 100 200 300 400 500k-i. ... 0.08. 0.10. Vol. atile. Fra. ctio. n. 0 Myrs 10 Myrs 100 Myrs 200 Myrs.

  4. MNRAS 000, 1–22 (2021) Preprint 29 September 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/yw23.pdf
    29 Sep 2023: Wyatt. 0 50 100 150 200 250 300 350. 20. 40. ... 0.01. 0 50 100 150 200 250 300 350. = 0.1.

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

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture16.pdf
    24 Nov 2023: e. e. 1.3 1.5. R 50!p. n. sR 200. FeR. 10. ... nuclei. (t 0.11s,. 1.3 1.5. R 50! Explosion (t 0.2s)sR 200.

  6. The clumpy structure of epsilon Eridani's debris disc revisited…

    https://people.ast.cam.ac.uk/~wyatt/bpkw23.pdf
    27 Mar 2023: MNRAS in press, 000–000 (2023). 8 M. Booth et al. 0 100 200 300Angle anti-clockwise from N, degrees. ... offs. et, ". C1. C2. C3 C4. C5. 0 100 200 300 400 500µJy/beam.

  7. MNRAS 000, 1–11 (2023) Preprint 31March 2023 Compiled…

    https://people.ast.cam.ac.uk/~wyatt/mmcb23.pdf
    31 Mar 2023: thisworkBolometricmagnitude (mag) 3.0020.0150.012 thiswork[Fe/H] 0.240.200.17 thiswork. ... parameters for the two components are determined byleast-squaresfitting to the observations.Wefind that the innerwarmcomponent has a best-fit temperature 𝑇warm

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