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
Gespeichert in:
| Hauptverfasser: | , , , , , , , , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2018
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| In: |
Monthly notices of the Royal Astronomical Society. Letters
Year: 2017, Jahrgang: 475, Heft: 1, Pages: L62-L66 |
| ISSN: | 1745-3933 |
| DOI: | 10.1093/mnrasl/slx184 |
| Online-Zugang: | Verlag, Volltext: https://doi.org/10.1093/mnrasl/slx184 Verlag, Volltext: https://academic.oup.com/mnrasl/article/475/1/L62/4705905 
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| Verfasserangaben: | Nathanial P. Hendler, Paola Pinilla, Ilaria Pascucci, Adriana Pohl, Gijs Mulders, Thomas Henning, Ruobing Dong, Cathie Clarke, James Owen, David Hollenbach |
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