activity
20032025
most citedChemical Processes in Protoplanetary Disks

211 citations · 1.1k across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.GA2025★ 1 cited

Isotopomer-Specific Carbon Isotope Ratio of Complex Organic Molecules in Star-Forming Cores

Ryota Ichimura, Hideko Nomura, Kenji Furuya +2

The recent observation of complex organic molecules (COMs) in interstellar ices by the James Webb Space Telescope (JWST), along with previous gas-phase detections, underscores the…

astro-ph.SR2020★ 14 cited

Chemical modelling of dust-gas chemistry within AGB outflows III. Photoprocessing of the ice and return to the ISM

M. Van de Sande, C. Walsh, T. J. Millar

To explain the properties of dust in the interstellar medium (ISM), the presence of a refractory organic mantle is necessary. The outflows of AGB stars are among the main contribut…

astro-ph.EP2018★ 22 cited

Candidate Water Vapor Lines to Locate the Snowline through High-dispersion Spectroscopic Observations. III. Submillimeter and Lines

Shota Notsu, Hideko Nomura, Catherine Walsh +4

In this paper, we extend the results presented in our former papers (Notsu et al. 2016, 2017) on using ortho- line profiles to constrain the location…

astro-ph.EP2016★ 43 cited

Candidate Water Vapor Lines to Locate the HO Snowline through High-Dispersion Spectroscopic Observations I. The Case of a T Tauri Star

Shota Notsu, Hideko Nomura, Daiki Ishimoto +4

Inside the HO snowline of protoplanetary disks, water evaporates from the dust-grain surface into the gas phase, whereas it is frozen out on to the dust in the cold region be…

astro-ph.SR2016★ 11 cited

Chemistry in AGB stars: successes and challenges

T. J. Millar

Emission and absorption line observations of molecules in late-type stars are a vital component in our understanding of stellar evolution, dust formation and mass loss in these obj…

astro-ph.SR2016★ 28 cited

ALMA-resolved salt emission traces the chemical footprint and inner wind morphology of VY CMa

L. Decin, A. M. S. Richards, T. J. Millar +6

(abreviated) We aim to study the inner-wind structure (R<250 Rstar) of the well-known red supergiant VY CMa. We analyse high spatial resolution (~0".24x0".13) ALMA Science Verifica…