Published in

Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S314(10), p. 207-208, 2015

DOI: 10.1017/s174392131500616x

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A Molecular Disk Survey of Low-Mass Stars in the TW Hya Association

This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Data provided by SHERPA/RoMEO

Abstract

AbstractWe have carried out an ALMA Cycle 2 survey of 15 confirmed or candidate low-mass (<0.2M) members of the TW Hya Association (TWA) with the goal of detecting line emission from CO molecular gas and continuum emission from cold dust. Our targets have spectral types of M4-L0 and hence represent the extreme low end of the TWA's mass function. The survey has yielded a detection of 12CO(2–1) emission around TWA 34. This newly discovered ~10 Myr-old molecular gas disk lies just ~50pc from Earth.

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