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26 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.

22 Mar 2024: evolutionary models. For example, Lovell et al. (2021) used ALMA to detect 4/30 Class III systems in the Lupus.

15 Apr 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.

10 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.

26 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;

19 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,

21 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

10 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

28 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.

12 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.