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Sub-millimetre non-contaminated detection of the disc around TWA7 by ALMA
(Oxford University Press, 2019)
Kinematic analysis and membership status of TWA22 AB
(EDP SCIENCES S A, 2009)
Context. TWA22 was initially regarded as a member of the TW Hydrae association (TWA). In addition to being one of the youngest (approximate to 8 Myr) and nearest (approximate to 20 pc) stars to Earth, TWA22 has proven to ...
Sub-millimetre non-contaminated detection of the disc around TWA 7 by ALMA
(2019)
Debris discs can be seen as the leftovers of giant planet formation and the possible nurseries of rocky planets. While M-type stars outnumber more massive stars we know very little about the time evolution of their ...
An ALMA survey for disks orbiting low-mass stars in the TW Hya Association
(EDP Sciences, 2015)
We carried out an ALMA survey of 15 confirmed or candidate low-mass (<0.2 M ) members of the TW Hya Association (TWA) with
the goal of detecting molecular gas in the form of CO emission, as well as of providing constraints ...
An ALMA survey for disks orbiting low-mass stars in the TW Hya Association
(EDP Sciences, 2015)
We carried out an ALMA survey of 15 confirmed or candidate low-mass (<0.2 M ) members of the TW Hya Association (TWA) with
the goal of detecting molecular gas in the form of CO emission, as well as of providing constraints ...
The TW Hydrae association: trigonometric paralaxes and kinematic analysis
(EDP SciencesLes Ulis, 2014)
Context. The nearby TW Hydrae association (TWA) is currently a benchmark for the study of the formation and evolution of young
low-mass stars, circumstellar disks, and the imaging detection of planetary companions. For ...
SSSPM J1102-3431 brown dwarf characterization from accurate proper motion and trigonometric parallax
(EDP SCIENCES S A, 2008)
Context. In 2005, Scholz and collaborators discovered, in a proper motion survey, a young brown dwarf SSSPM J1102-3431 (SSSPM J1102) of spectral type M8.5, probable member of the TW Hydrae Association and possible companion ...