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1 - 10 of 14 search results for katalk:za33 24 |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. Carolin Crawford

    https://people.ast.cam.ac.uk/~csc/cv.html
    15 Feb 2021: Public Outreach Talks. Synopses, videos, powerpoints and transcripts are available for my 24 Gresham lectures and my two Darwin College lectures are available from YouTube and also here.

  3. Publications list for Carolin Crawford

    https://people.ast.cam.ac.uk/~csc/newcv/Full%20publications%20list%20for%20Carolin%20Crawford.pdf
    15 Feb 2021: 24. Fabian AC, Sanders JS, Taylor GB, Allen SW, Crawford CS, Johnstone RM, Iwasawa K 2006 MNRAS 366 417-428 A very deep Chandra observation of the Perseus cluster: shocks, ripples ... 10. Crawford CS 2007 The Reader , no 24, p 50-52 Heavenly Inspiration.

  4. Publications list for Carolin Crawford

    https://people.ast.cam.ac.uk/~csc/newcv/Recent%20publications%20list%20for%20Carolin%20Crawford.pdf
    15 Feb 2021: 10. Crawford CS 2007 The Reader , no 24, p 50-52 Heavenly Inspiration.

  5. Carolin Crawford - Outreach Talks

    https://people.ast.cam.ac.uk/~csc/talksyn.html
    15 Feb 2021: Short abstracts, video recordings, a copy of the slides and a transcript are available for all 24 of my Gresham lectures, at a dedicated Gresham College website..

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

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture10.pdf
    16 Nov 2021: the H-R diagram). Recallingthat:. L = 4πR2 σT 4eff (10.25). we obtain, combining 10.25, 10.18 and 10.24:. ... Using eq. 10.16 together with our mass-radius relation(10.24), we have:. T =µmHk.

  7. MNRAS 000, 1–15 (2020) Preprint 29April 2021 Compiled…

    https://people.ast.cam.ac.uk/~wyatt/ckkm21.pdf
    29 Apr 2021: MNRAS 000, 1–15 (2020) Preprint 29April 2021 Compiled usingMNRASLATEXstyle file v3.0. ALMA imaging of the M-dwarf Fomalhaut C’s debris disc. Patrick F.Cronin-Coltsmann,1,2 GrantM.Kennedy,1,2 PaulKalas,3,4,5JulienMilli,6,7 Cathie J. Clarke,8

  8. Draft v17Preprint typeset using LATEX style emulateapj v. 12/16/11 ...

    https://people.ast.cam.ac.uk/~wyatt/dhks21.pdf
    8 Mar 2021: 2. LBTI OBSERVATIONS OF β LEO. 2.1. Instrument Setup. Observations of β Leo were acquired with the LargeBinocular Telescope Interferometer (LBTI) on April 24,2013 in L’ band (3.41 - ... These constraints are the observed 24-µm ex-cess of 37%, a 40%

  9. Publications of the Astronomical Society of Australia (PASA)doi:…

    https://people.ast.cam.ac.uk/~wyatt/khna21.pdf
    23 Nov 2021: P.20,36, Larsson,B.21, McClure, M.22, Miotello, A.23 Momose, M.24, Nakagawa, T.15, Naylor, D.25, Nisini, B.26,Notsu, S.27, Onaka, T.28,8,

  10. MNRAS 000, 1–23 (2020) Preprint 14 June 2021 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/lmwk21.pdf
    16 Jul 2021: Orbit F606W1 [s] F606W2 [s] Roll []. 1 540 (x4) = 2160 575 (x4) = 2300 0.02 540 (x4) = 2160 575 (x4) = 2300 24.9. ... 24 4.790.23 magH g 1.65 4.400.23 magKS g 2.16 4.340.28 mag.

  11. MNRAS 000, 1–27 (2020) Preprint 27October 2020 Compiled…

    https://people.ast.cam.ac.uk/~wyatt/lwak20.pdf
    10 Feb 2021: Young Stellar Objects (YSOs) in star forming regions can beclassified based on theirmid-infrared emission (e.g., 24 𝜇m). ... Six of the class II sources are found to have 𝛼IR < 1.6 if12 𝜇m is used instead of 24 𝜇m.

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