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

    https://people.ast.cam.ac.uk/~wyatt/bpkw23.pdf
    27 Mar 2023: Observations over multipleepochs are necessary to test whether the observed features rotate around the star. ... We first test this processwith the original unsmoothed data and confirm that we mea-.
  3. M. Pettini: Structure and Evolution of Stars — Lecture ...

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture16.pdf
    24 Nov 2023: This is fundamental work, providing empirical tests ofour theories of stellar evolution for massive stars. ... Middle pair: SN2005cs in M51 ata distance of 7 Mpc. Bottom pair: SN2003gd in the face-on spiral galaxy M74 at adistance of 9 Mpc.
  4. MNRAS 000, 1–16 (2022) Preprint 6 July 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/bwmd23.pdf
    11 Jul 2023: ted lines) at various epochs. The middle panel shows the volatilecontent of planetesimals as a function of diameter. ... order of magnitude.This is plausibly an important test of whether large planetes-imals.

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