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Prof Richard McMahon, Institute of Astronomy, Cambridge Home Page
https://people.ast.cam.ac.uk/~rgm/28 Jun 2024: Strabane had moved out of the top 20 in the 2008 edition.". -
Erin E Hayes
https://people.ast.cam.ac.uk/~eeh55/resume.html2 May 2024: Presented “The Fate of the Universe” talk to three groups of 20 Year 5 (Ages 9-10) students. -
Astronomy & Astrophysics manuscript no. aa ©ESO 2024April 9, ...
https://people.ast.cam.ac.uk/~wyatt/ylkw24.pdf9 Apr 2024: 0. 20. 40. 60. 80. 100. Inte. nsity. (%). ALMA-NEALMA-SWHerschel70-NEHerschel70-SWmodel profile-ALMA beammodel profile-Herschel70 beamALMA beam sizeHerschel70 beam size. ... Using equation (20)in Wyatt et al. (2007) and assuming the warm component -
Draft version July 18, 2022Typeset using LATEX default style ...
https://people.ast.cam.ac.uk/~wyatt/swmw22.pdf22 Mar 2024: 2010), the Spitzer 70 µm observations of a subsample of 20 systems (red, Stauffer et al. ... µm (20′′) clearly encompass any circumstellar dust emission around Pleiades members but also raise the spectre of. -
Quanz_et_al_ESA_white_paper_MIR_interferometry_revised
https://people.ast.cam.ac.uk/~wyatt/qabb22.pdf22 Mar 2024: Figure 1: Molecules relevant to terrestrial planet characterization between 3-20 μm (adapted from Catling et al. ... In the following we will summarize what developments from ground and space we can expect in the coming 20 years. -
Cosmic dust fertilization of glacial prebiotic chemistry on early ...
https://people.ast.cam.ac.uk/~wyatt/wrll24.pdf22 Mar 2024: Nonetheless, even Dry Valleys type cryoconite deposits are subject to transportthrough ice dynamics of up to 20 m/yr [41], precluding long-term formations. ... Origins of Life and Evolution of Biospheres 38, 5–21(2008). [20] Maurette, M., Hammer, C., -
2-3, D-07745 Jena, GermanyDraft version February 14, 2023Typeset…
https://people.ast.cam.ac.uk/~wyatt/mbpw22.pdf22 Mar 2024: to 20 Micron Spectrum of the Planetary-Mass Companion VHS 1256-1257 b. ... MIRI Channel 4, Short A 17.71 - 20.94 FULL FASTR1 1,460 – 1,930 1576.22. -
MNRAS 000, 1–17 (2023) Preprint 25 October 2023 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/ckkl23.pdf22 Mar 2024: The 𝛽 PictorisMoving Group (BPMG) is both young (20 Myr, Bell et al. ... 36 0.908 -V WW PsA 35 20 78 0.908 -AU Mic - 110 13000 - 40. -
MNRAS 000, 1–17 (2033) Preprint 19 June 2023 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/tmbh23.pdf22 Mar 2024: ph.E. P] 1. 6 Ju. n 20. 23. 2 James Terrill et al. ... 𝜎𝑟 (au) ⟨𝑖⟩ (). 0.01 5 89.31.00.50.01 10 89.21.20.20.01 20 89.61.20.40.03 5 89.61.30.50.03 10 -
Astronomy & Astrophysics manuscript no. SHARDDS ©ESO 2022August…
https://people.ast.cam.ac.uk/~wyatt/dmac22.pdf22 Mar 2024: This detection rate re-quires the successive injection of 20 fake companions per con-sidered annulus. ... We relied on ten particles with a maximum number ofiterations equal to 20. -
Inner edges of planetesimal belts: collisionally eroded or truncated?
https://people.ast.cam.ac.uk/~wyatt/immb23.pdf20 Feb 2024: Accepted 2023 April 21. Received 2023 April 20; in original form 2022 September 9. ... nloaded from https://academ. ic.oup.com/m. nras/article/522/4/6150/7143114 by guest on 20 February 2024. -
Draft version March 24, 2022Typeset using LATEX twocolumn style ...
https://people.ast.cam.ac.uk/~wyatt/hycd22.pdf22 Mar 2024: 20. 30. Du. st-t. o-G. asR. atio. Gas Density. Dust Density. ... The dusttemperature also affects the timescales relevant for grainalignment, but the 20% difference is inconsequential (seeSection 8). -
MNRAS 000, 1–14 (2022) Preprint 18 January 2023 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/hwd22.pdf22 Mar 2024: 7 Ja. n 20. 23. 2 Han et al. depends on the relative fractions of planetesimals in each differenttype of resonance (Wyatt 2003). ... Median 1𝜎 2𝜎 3𝜎. Linear displacement speed (au/yr) 0.018 (-0.099, 0.13) (-0.29, 0.33) (-0.86, 0.90)Location atMJD -
Astronomy & Astrophysics manuscript no. main ©ESO 2023October 11, …
https://people.ast.cam.ac.uk/~wyatt/dmch23.pdf22 Mar 2024: 5 10 15 20. Distance from the Sun (pc). 0.2. 0.4. ... 5. 10. 15. 20. 25. MK. 1(m. ag). (1). (3). M0-M5. -
DRAFT VERSION JULY 17, 2023Typeset using LATEX twocolumn style ...
https://people.ast.cam.ac.uk/~wyatt/srw23.pdf22 Mar 2024: 2018; Wyatt2020). To date, such exo-Kuiper belts, or debris disks, havebeen detected around 20% of nearby main-sequence starsthrough their excess emission at infrared wavelengths (Mon-tesinos et al. ... with a power-law in-dex of p = 1 with ain = 30 au -
MNRAS 000, 1–17 (2022) Preprint 28 June 2022 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mcjm22.pdf22 Mar 2024: ph.E. P] 2. 7 Ju. n 20. 22. 2 S. Marino. ... 𝑅ion,0 =. 𝜙𝜆𝜎CI d𝜆, (20). andcorrespondstoanionisationtimescaleof100yr.Recombinationis calculated as. 𝑅rc(𝑧) = 𝛼rc(𝑇)𝑛e (𝑧), (21). -
MNRAS 000, 1–24 (2023) Preprint 9 November 2023 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/pksj23.pdf22 Mar 2024: such dust is detected around 20% of main-sequence stars(Hughes et al. ... Each simulation comprises one star, one planet,and a disc of 20,000 massless debris particles.
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