most citedIPA. Accretion rate of a low-mass Class 0 protostar, measured via mid-infrared fluorescent OH emission

1 citations · 1 across the 6 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2026

The Structure and Kinematics of Three Class 0 Protostellar Jets from JWST

Samuel A. Federman, S. Thomas Megeath, Alessio Caratti o Garatti +20

We present observations of jets within 2000 au of three deeply embedded protostars using 2.9-27 micron observations with JWST. These observations show the morphologies and kinemati…

astro-ph.SR20251 cited

IPA. Accretion rate of a low-mass Class 0 protostar, measured via mid-infrared fluorescent OH emission

Dan M. Watson, Mayank Narang, Caeley V. Pittman +41

The earliest stages of star formation are highlighted by complex interactions between accretion, outflow, and radiative processes, which shape the chemical and physical environment…

astro-ph.IM2025

Sub-millimeter wavelength protostellar accretion rate monitoring with AtLAST

Thomas Stanke, Verena Wolf, Bringfried Stecklum +5

How a star forms is a fundamental question in astrophysics. In the earliest stages of protostellar evolution high extinction prevents a direct study of the accretion processes and…

astro-ph.IM2025

Serendipitous and targeted mm/sub-mm transient searches with wide-FOV telescope

Karri Koljonen, Claudio Ricci, Thomas Stanke +4

The millimeter/sub-millimeter (mm/sub-mm) sky remains a rich but under-explored frontier for transient and variable phenomena. A wide-field, high-sensitivity instrument with a larg…

astro-ph.GA2025

Mass Assembly and Chemical Complexity in the Milky Way

Pamela Klaassen, David Eden, Alessio Traficante +13

(Sub-)millimeter spectral lines can be used not only to understand the chemical complexity and enrichment history of an observed portion of our Galaxy, but with spectrally resolved…

astro-ph.GA2025

Dust scattering halo of 4U 1630-47: High resolution X-ray and mm observations constrain source and molecular cloud distances

E. Kalemci, M. Díaz Trigo, E. Oztaban +8

We re-investigated the distance to the black hole X-ray binary 4U 1630-47 by analyzing its dust scattering halo (DSH) using high-resolution X-ray (Chandra) and millimeter (APEX) ob…