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From the 1 of 10 linked papers with an AI index.

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10 papers

astro-ph.SR2026

JWST/MIRI Detection of Molecular H Winds from an Edge-on Class II Source HV Tau C

Vinod Chandra Pathak, P. Manoj, Himanshu Tyagi +14

The paper uses JWST/MIRI mid‑infrared spectroscopy to detect and characterize a wide‑angled molecular hydrogen wind from the edge‑on Class II protoplanetary disk HV Tau C, measurin…

astro-ph.SR2026

Far-ultraviolet flux distribution in Orion and its relation to stellar accretion

Rossella Anania, Andrew J. Winter, Miguel Vioque +8

Orion is the closest region hosting active star formation and young OBA stars. Computing far-ultraviolet (FUV) fluxes at its stars is essential to connect stellar and protoplanetar…

astro-ph.GA2026

Probing outflow physics through CHCN and CHOH chemistry

L. Giani, D. Zaremba, M. De Simone +4

Chemical correlations between molecules provide powerful diagnostics to probe the physical conditions of protostellar outflows. In particular, the relationship between methanol (CH…

astro-ph.EP2026

MINDS: Complementary inclinations in the binary system HK Tau reveal gas- and ice-phase chemistry

Alice Somigliana, Giulia Perotti, Nicolás T. Kurtovic +18

[Abridged] HK Tau is a roughly equal mass pre-main sequence binary system consisting of a low-inclination primary (57 deg) and an edge-on (83 deg) secondary. We present JWST/MIRI o…

astro-ph.SR2026

MINDS survey of silicates in T Tauri disks: Correlation between dust and gas

J. Varga, Th. Henning, L. B. F. M. Waters +20

Context. Silicates are key constituents of planet-forming disks and major building blocks of rocky planets. Mid-infrared spectral features of micron-sized silicate grains trace gra…

astro-ph.SR2026

The Accretion Process on Protostars

Eleonora Fiorellino, Alice Somigliana

The process of mass accretion onto Young Stellar Objects (YSOs) plays a fundamental role in determining the final stellar mass and setting the initial conditions for planet formati…