A likely planet-induced gap in the disc around T Cha

Abstract. We present high-resolution (0.11 × 0.06 arcsec2) 3 mm ALMA observations of the highly inclined transition disc around the star T Cha. Our continuum i

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Bibliographic Details
Main Authors:	Hendler, Nathanial P. (Author) , Pinilla, Paola (Author) , Pascucci, Ilaria (Author) , Pohl, Adriana (Author) , Mulders, Gijs (Author) , Henning, Thomas (Author) , Dong, Ruobing (Author) , Clarke, Cathie (Author) , Owen, James (Author) , Hollenbach, David (Author)
Format:	Article (Journal)
Language:	English
Published:	2018
In:	Monthly notices of the Royal Astronomical Society. Letters Year: 2017, Volume: 475, Issue: 1, Pages: L62-L66
ISSN:	1745-3933
DOI:	10.1093/mnrasl/slx184
Online Access:	Verlag, Volltext: https://doi.org/10.1093/mnrasl/slx184 Verlag, Volltext: https://academic.oup.com/mnrasl/article/475/1/L62/4705905
Author Notes:	Nathanial P. Hendler, Paola Pinilla, Ilaria Pascucci, Adriana Pohl, Gijs Mulders, Thomas Henning, Ruobing Dong, Cathie Clarke, James Owen, David Hollenbach

Description
Summary:	Abstract. We present high-resolution (0.11 × 0.06 arcsec2) 3 mm ALMA observations of the highly inclined transition disc around the star T Cha. Our continuum i
Item Description:	Advance access publication 2017 December 6 Gesehen am 24.09.2019
Physical Description:	Online Resource
ISSN:	1745-3933
DOI:	10.1093/mnrasl/slx184