collaborators

7 papers

astro-ph.SR2026

The Preliminary Mauve Science Programme: Science themes identified for the first year of operations

Mauve Science Collaboration, Marcel Agueros, Don Dixon +22

Mauve is a low-cost small satellite developed and operated by Blue Skies Space Ltd. The payload features a 13 cm telescope connected with a fibre that feeds into a UV-Vis spectrome…

astro-ph.GA2025

PROJECT-J: the shocking H2 outflow from HH46

Maria Gabriela Navarro, Brunella Nisini, Teresa Giannini +14

We analyze the H2 emission observed in the HH46 Class I system as part of PROJECT-J (Protostellar Jets Cradle Tested with JWST), to investigate the origin and excitation of the war…

astro-ph.SR2025

Coordinated Space- and Ground-based Monitoring of Accretion Bursts in a Protoplanetary Disk: The Orbital and Accretion Properties of DQ Tau

Hala Alqubelat, Carlo F. Manara, Justyn Campbell-White +9

Multiplicity in pre-main-sequence (PMS) systems shapes circumstellar and circumbinary disks, often producing features such as inner cavities, spiral arms, and gas streamers that fa…

astro-ph.SR2025

Variability of the DG Tau Forbidden Emission Line Low Velocity Component

Noah Otten, Emma Whelan, Yu-Ru Chou +3

Optical Forbidden Emission Lines (FELs) come from transitions with long radiative decay times needing low density gas where collisions between atoms are rare. They are produced in…

astro-ph.SR2025

Coordinated Space and Ground-Based Monitoring of Accretion Bursts in a Protoplanetary Disk: Establishing Mid-Infrared Hydrogen Lines as Accretion Diagnostics for JWST-MIRI

Benjamin M. Tofflemire, Carlo F. Manara, Andrea Banzatti +17

In this paper, we establish and calibrate mid-infrared hydrogen recombination lines observed with JWST as accretion tracers for pre-main-sequence stars that accrete from circumstel…

astro-ph.SR2025

A Spectroastrometric Study of the Low-velocity Wind from DG Tau A

Yu-Ru Chou, Michihiro Takami, Shin-Ping Lai +9

We obtained high spectral resolution spectra ( 2.5 km s) for DG Tau A from 4800 Ã to 7500 Ã using Subaru High Dispersion Spectrograph (HDS) for the first time. T…