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Draft version February 20, 2021Typeset using LATEX default style ...
https://people.ast.cam.ac.uk/~wyatt/wgml21.pdf19 Jul 2021: 2. SpiKeS 7. ¡0:10. ¡0:05. 00:05. 0:100. 20. 40. 60. 80. ... 8 Werner et al. 2 pixel radius and a sky annulus from 12 to 20 pixels. -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture10.pdf16 Nov 2021: 2. (T)β(10.20). We also have:. T P. ρ, T M. 2. ... 0.20 (1 0.7). M. M. ' 3.8 104 MM. (10.41). 12. -
Publications list for Carolin Crawford
https://people.ast.cam.ac.uk/~csc/newcv/Full%20publications%20list%20for%20Carolin%20Crawford.pdf15 Feb 2021: 20. Crawford CS 1993 In Observing at a Distance eds. Emerson DT, Clowes RG,; World Scientific Publishing, p305-307 Remote observing in Edinburgh - a first-time user's view. ... 20. Fabian AC, Crawford CS, Forbes, DA, Johnstone RM 1989, Gemini, 26, 6-7 -
MNRAS 000, 1–6 (2020) Preprint 30November 2020 Compiled…
https://people.ast.cam.ac.uk/~wyatt/lkmw20.pdf10 Feb 2021: 2 NO LUP IN CONTEXT. NO Lup (2MASS J160311.8-323920) is located in Cloud I of Lu-pus at 𝛼=16:03:11.812, 𝛿=-32:39:20.31 (J2000) ... blackbody planetesimal belt radius as 𝑅BB=3.20.3au, seeLovell et al. -
arX iv:2 110. 0431 9v1 [as tro- ph.E P] ...
https://people.ast.cam.ac.uk/~wyatt/wyat21.pdf12 Oct 2021: However, this still means that it is onlythe brightest 20% of exozodi that have been detected, and inferences about lower dust levels have to begleaned by extrapolation. ... However, it is already clear that for 20% of stars, thelevel of dust in their -
Quanz_et_al_ESA_white_paper_MIR_interferometry_revised
https://people.ast.cam.ac.uk/~wyatt/qabb21.pdf20 Aug 2021: 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. -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture04.pdf7 Oct 2021: 90-120Jan 19 3754.9015 3755.2006 33 100-130Jan 20 3755.9245 3756.1993 25 90-120Jan 21 3756.9068 3757.0386 14 60-150Jan 22 3757.9004 3758.1621 -
CO gas from the aftermath of a giant impact ...
https://people.ast.cam.ac.uk/~wyatt/smjk21.pdf10 Nov 2021: This makes the presence of CO, a. highly volatile gas with sublimation temperatures as low as 20 K, extremely surprising in a. ... around a large cavity. arXiv 853, 162 (2017). 20. Morris, M. -
Publications of the Astronomical Society of Australia (PASA)doi:…
https://people.ast.cam.ac.uk/~wyatt/khna21.pdf23 Nov 2021: Furthermore, ALMA surveys. HD (1-0) [W m-2]10 -20 10 -19 10 -18. ... The low excitationHD lines, J = 1 0, J = 2 1, are expected to havetypical widths of 5 20 km/s, dependent also on inclina-tion. -
MNRAS 000, 1–15 (2020) Preprint 29April 2021 Compiled…
https://people.ast.cam.ac.uk/~wyatt/ckkm21.pdf29 Apr 2021: 2013); itwas not spatially resolvedbut a temperature of 24K and radius of 20-40 auwere estimated. ... Δ𝜒2 0 2 20. ΔBIC 0 42 40. 6” 4” 2” 0” -2” -4” -6”RA Offset. -
MNRAS 000, 1–23 (2021) Preprint 1December 2021 Compiled…
https://people.ast.cam.ac.uk/~wyatt/rw21.pdf2 Dec 2021: We define JFCs to have periods 𝑃 < 20 yr and a Tisserandparameter with respect to Jupiter of 2 < 𝑇𝐽 < 3 as in Nesvornýet al. ... 0. 20. 40. 60. 80. 100Su. rviv. al fr. acti. on (. %). Figure 4. Fraction of cometswhich survive their dynamical -
MNRAS 000, 1–27 (2020) Preprint 27October 2020 Compiled…
https://people.ast.cam.ac.uk/~wyatt/lwak20.pdf10 Feb 2021: N. Background. Class III. Observed Class III. Observed Class II. 40 20 0 20 40µα [mas/yr]. ... 20 40 30 40Sz107 - - < 60 - - - - - - -. J155526.2-333823 7.58 0.10 - - 80 15 3.3 1.5 3.8 0.8 31 12 138 21 30 60 90 50. -
MNRAS 000, 1–23 (2020) Preprint 14 June 2021 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/lmwk21.pdf16 Jul 2021: We note that there are two 850 𝜇m flux measurements, ourALMAdata (13.21.3mJy) and JCMTdata (20.12.7mJy). ... 20′′ | 101.83.5auWidth (𝑊HM) Major 2.490.22′′ | 434auPeakBrightness Major 0.2170.009mJyarcsec1PeakBrightness Minor
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