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Mark Wyatt
https://people.ast.cam.ac.uk/~wyatt/17 Jul 2024: The effect of stellar multiplicity on protoplanetary discs. A NIR survey of the Lupus star forming region.. ... ALMA Survey of Lupus Class III Stars: Early Planetesimal Belt Formation and Rapid Disk Dispersal. -
MNRAS 000, 1–11 (2020) Preprint 26November 2020 Compiled…
https://people.ast.cam.ac.uk/~wyatt/zcac20.pdf26 Nov 2020: Only 4 multiple systems in Lupus have all the componentsdetected also by ALMA. ... 4 Results. 5 Discussion. 6 Summary and conclusions. A Not observable Lupus objects. -
MNRAS 000, 1–6 (2020) Preprint 30November 2020 Compiled…
https://people.ast.cam.ac.uk/~wyatt/lkmw20.pdf10 Feb 2021: A recent ALMA survey of class III stars in Lupus founddust in several systemswithdustmasses orders ofmagnitude lowerthan protoplanetary disc levels and consistent with originatingin the progenitors of debris discs seen at -
arX iv:2 110. 0431 9v1 [as tro- ph.E P] ...
https://people.ast.cam.ac.uk/~wyatt/wyat21.pdf12 Oct 2021: van Terwisga. ALMA Survey of Lupus Protoplanetary Disks. I. Dust and Gas Masses. ... P. Williams. ALMA survey of Lupus class III stars: Earlyplanetesimal belt formation and rapid disc dispersal. -
MNRAS 000, 1–27 (2020) Preprint 27October 2020 Compiled…
https://people.ast.cam.ac.uk/~wyatt/lwak20.pdf10 Feb 2021: MNRAS 000, 1–27 (2020). ALMA Survey of Lupus Class III stars 3. ... MNRAS 000, 1–27 (2020). ALMA Survey of Lupus Class III stars 5. -
lecture3_extrasolarplanets
https://people.ast.cam.ac.uk/~wyatt/lecture3_extrasolarplanets.pdf28 Jan 2009: GQ Lup: 0.7Msun K7eV a 0.1-2Myr in Lupus with a 10-20MJ companion at 98 AU, high Hα indicates possibly still accreting (Neuhauser et al. -
Draft version July 18, 2022Typeset using LATEX default style ...
https://people.ast.cam.ac.uk/~wyatt/swmw22.pdf22 Mar 2024: evolutionary models. For example, Lovell et al. (2021) used ALMA to detect 4/30 Class III systems in the Lupus. -
MNRAS 000, 000–000 (2018) Preprint 21 February 2019 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mphp19.pdf21 Feb 2019: 2012; Boneberg et al. 2016).Using ALMA data, a recent survey of the Lupus star form-ing region gives evidence that supports low observed g/d inprotoplanetary discs; Miotello et al. ... For comparison, in an ALMA survey of Lupus, mostlow-mass discs have a -
Publications of the Astronomical Society of Australia (PASA)doi:…
https://people.ast.cam.ac.uk/~wyatt/khna21.pdf23 Nov 2021: dust masses have been measured in five star formingregions (Taurus, Lupus, Chameleon I, Upper Sco andCorona Australis, from Andrews et al., 2013; Ansdellet al., 2016; Barenfeld et al., 2016; Pascucci et -
Mon. Not. R. Astron. Soc. 000, 1–23 (2002) Printed ...
https://people.ast.cam.ac.uk/~wyatt/kmwk18.pdf22 Nov 2018: 2016a,b) that is proba-bly a member of the Upper Centaurus Lupus moving group(a subgroup of the Sco-Cen association, Rizzuto et al. -
Mon. Not. R. Astron. Soc. 000, 1–23 (2012) Printed ...
https://people.ast.cam.ac.uk/~wyatt/jw12.pdf19 Jun 2012: Mon. Not. R. Astron. Soc. 000, 1–23 (2012) Printed 18 June 2012 (MN LATEX style file v2.2). Debris from terrestrial planet formation: the Moon-forming collision. Alan P. Jackson1? and Mark C. Wyatt1?1Institute of Astronomy, University of Cambridge, -
arX iv:1 709. 0841 4v1 [as tro- ph.S R] ...
https://people.ast.cam.ac.uk/~wyatt/mcka17.pdf26 Sep 2017: Column (4): Luminosity. Column (5): Moving group membership. ARG: Argus moving group;BPMG: β Pic moving group; COL: Columba moving group; LCC: Lower Centaurus Crux association; UCL: Upper Centaurus Lupus association; -
MNRAS 433, 2334–2356 (2013) doi:10.1093/mnras/stt900Advance Access…
https://people.ast.cam.ac.uk/~wyatt/kw13.pdf16 Jul 2013: Centaurus Crux(LCC), Upper Centaurus Lupus (UCL) and Upper Scorpius (US)(i.e.
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