Search
Search Funnelback University
- Refined by:
- Date: Past month
1 -
10 of
15
search results for TALK:PC53 20 |u:people.ast.cam.ac.uk
where 0
match all words and 15
match some words.
Results that match 1 of 2 words
-
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. -
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 -
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., -
Mark Wyatt
https://people.ast.cam.ac.uk/~wyatt/15 Apr 2024: The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems II: A 1 to 20 Micron Spectrum of the Planetary-Mass Companion VHS1256-1257b. -
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. -
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).
Refine your results
clear all
Date
Search history
Recently clicked results
Recently clicked results
Your click history is empty.
Recent searches
Recent searches
Your search history is empty.