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20242026
most citedOGHReS: Star formation in the Outer Galaxy (-)

13 citations · 24 across the 6 of their papers we have counts for

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6 papers · 1 filter

astro-ph.GA2026

From DES to KiDS: Domain adaptation for cross-survey detection of low-surface-brightness galaxies

Hareesh Thuruthipilly, Krzysztof Lisiecki, Junais +19

Low-surface-brightness galaxies (LSBGs) are vital for understanding galaxy formation, but their diffuse nature makes them challenging to detect. Upcoming large-scale surveys are ex…

astro-ph.GA2025

A multiscale evolutionary study of molecular gas in STARFORGE. I. Synthetic observations of SEDIGISM-like molecular clouds

K. R. Neralwar, D. Colombo, S. Offner +6

Molecular clouds are active sites of star formation in galaxies, and their formation and evolution are largely affected by stellar feedback. This includes outflows and winds from n…

astro-ph.GA2025★ 5 cited

UV-irradiated outflows from low-mass protostars in Ophiuchus with JWST/MIRI

I. M. Skretas, A. Karska, L. Francis +7

The main accretion phase of protostars is characterized by the ejection of material in the form of jets/outflows. External UV irradiation can potentially have a significant impact…

astro-ph.GA2025★ 3 cited

OGHReS: Star formation in the Outer Galaxy II (-)

J. S. Urquhart, C. Koenig, D. Colombo +19

The Outer Galaxy High-Resolution Survey (OGHReS) covers 100 square degrees () in the (2--1) transitions of three CO-isotopologues. We use the spectra…

astro-ph.GA2025★ 3 cited

SOFIA FIFI-LS spectroscopy of DR21 Main: energetics of the spatially-resolved outflow from a high-mass protostar

A. Karska, M. Figueira, A. Mirocha +12

Massive star formation is associated with energetic processes that may influence the physics and chemistry of parental molecular clouds and impact galaxy evolution. The high-mass p…

astro-ph.GA2024★ 13 cited

OGHReS: Star formation in the Outer Galaxy (-)

J. S. Urquhart, C. König, D. Colombo +11

We have used data from the Outer Galaxy High-Resolution Survey (OGHReS) to refine the velocities, distances, and physical properties of a large sample of 3584 clumps detected in fa…