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21 - 30 of 33 search results for news |u:people.ast.cam.ac.uk

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  2. MNRAS 000, 1–17 (2023) Preprint 25 October 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/ckkl23.pdf
    22 Mar 2024: An ALMA Survey of M-dwarfs in the Beta Pictoris Moving Group withTwo New Debris Disc Detections. ... 2018),further solidifying the BPMG as a good candidate sample to searchfor new discs.

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

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture07.pdf
    23 Oct 2023: Tb. Ho. Er. Tm. Yb. Hf. Dy. Figure 1.— Recent abundance determinations in five r-process rich stars, based upon new atomiclab data, compared with two solar system r-process only

  4. Astronomy & Astrophysics manuscript no. SHARDDS ©ESO 2022August…

    https://people.ast.cam.ac.uk/~wyatt/dmac22.pdf
    22 Mar 2024: Large surveys provided new insights about the frequency and properties of massive sub-stellar companions withseparations from 5 to 300 au.Aims. ... A new planetary characterisation algorithm, based on the RSM framework, is developed and testedsuccessfully

  5. MNRAS 000, 1–17 (2022) Preprint 28 June 2022 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mcjm22.pdf
    22 Mar 2024: In 2 we present and describe a new model thattakes into account photodissociation, vertical diffusion, ionisation,and viscous evolution of gas continuously released in a planetesi-mal belt.

  6. Inner edges of planetesimal belts: collisionally eroded or truncated?

    https://people.ast.cam.ac.uk/~wyatt/immb23.pdf
    20 Feb 2024: 2018 ; Marino 2021 ), we include a new dataet with a higher resolution (0.2 arcsec = 5 au) from an unfinishedycle 7 program (2019.1.00189.S). ... This new data set is described inppendix A. Finally, for HR 8799 and HD 107 146 we subtract emission from.

  7. 2-3, D-07745 Jena, GermanyDraft version February 14, 2023Typeset…

    https://people.ast.cam.ac.uk/~wyatt/mbpw22.pdf
    22 Mar 2024: 9Department of Astrophysics, American Museum of Natural History, Central Park West at 79th St., New York, NY 10024, USA10Space Telescope Science Institute, 3700 San Martin Dr., Baltimore, MD 21218, USA.

  8. Draft version March 24, 2022Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/hycd22.pdf
    22 Mar 2024: Draft version March 24, 2022Typeset using LATEX twocolumn style in AASTeX63. Polarization from Aligned Dust Grains in the β Pic Debris Disk. Charles L. H. Hull ,1, 2, Haifeng Yang (杨海峰) ,3, 4 Paulo C. Cortés ,5, 2 William R. F. Dent,6, 2.

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

    https://people.ast.cam.ac.uk/~wyatt/bwmd23.pdf
    11 Jul 2023: 2018, e.g. cometC/2016 R2)). The recent New Horizons fly-by of Arrokothplaced upper limits on the release of hyper-volatiles (CO,. ... Jutzi & Benz 2017; Davidsson 2023).Collisions also expose new surface, such that volatiles canbe lost via sublimation

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

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture16.pdf
    24 Nov 2023: 16.1 A Little History. In 1572 the Danish astronomer Tycho Brahe observed a new star in theconstellation of Cassiopeia and described it in his book De Stella Nova(Latin for ... Concerning the New Star”), giving rise to the name nova.Novae are now

  11. DRAFT VERSION JULY 17, 2023Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/srw23.pdf
    22 Mar 2024: Recently, thanks to the advent of new generation instru-ments such as ALMA, it has become possible to imagetens of debris disks with high angular resolution at millime-ter wavelengths. ... As we show below, even at this level of approximation,

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