On the methanol emission detection in the TW Hya disc: the role of grain surface chemistry and non-LTE excitation

Research output: Contribution to journal › Article › peer-review

Original language	English
Pages (from-to)	2024-2031
Number of pages	8
Journal	Monthly Notices of the Royal Astronomical Society
Volume	468
Issue number	2
DOIs	https://doi.org/10.1093/mnras/stx624
Publication status	Published - Jun 2017

astrochemistry, line:formation, molecular processes, protoplanetary discs, stars:individual:TW Hya, submillimetre:planetary systems., TURBULENT PROTOPLANETARY DISKS, SOLAR NEBULA, PLANET FORMATION, 1ST DETECTION, HYDRAE, LINE, GAP, EVOLUTION, DUST, CO

ID: 1809086