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From the 1 of 23 linked papers with an AI index.

activity
20242026
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23 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.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.EP2026

Implications of self-consistent HO ice optical constants on radiative transfer models of disks

Z. L. Smith, M. K. McClure, I. Kamp +1

Interstellar water (HO) ice exhibits significantly varied profiles over its spectral features with temperature and thermal history. No previous radiative transfer model of a pr…

astro-ph.EP2026

Chemistry and IR emission of acetylene in planet-forming regions of T Tauri disks. Impact of elemental abundances and dust properties

Pacôme Estève, Benoît Tabone, Emilie Habart +5

(Abridged) We aim to explore the parameters that influence the mid-infrared emission of CH and HO, and if the spread observed in / is tr…

astro-ph.EP2026

Geophysical and atmospheric implications of O-dependent melting on rocky exoplanets

Mariana Sastre, Tim Lichtenberg, Laurent Soucasse +3

The geochemical evolution of long-lived magma oceans is strongly regulated by volatile exchange between the molten mantle and the atmosphere. For planets inside the runaway-greenho…

astro-ph.SR2026

Improving Accretion Diagnostics for Young Stellar Objects with Mid-infrared Hydrogen lines from JWST/MIRI

B Shridharan, P Manoj, Vinod Chandra Pathak +10

We present a comprehensive study of mid-infrared neutral hydrogen (H~\textsc{i}) emission lines in 79 nearby (d 200 ) young stars using JWST/MIRI. We aim to identify mid-in…