activity
20242026
collaborators

8 papers

astro-ph.SR2026

Dynamical masses of young stellar objects with the VLBA: DYNAMO-VLBA: Radio binary stars in Orion

Sergio A. Dzib, Jazmín Ordóñez-Toro, Laurent Loinard +9

We present results from a multi-epoch Very Long Baseline Array (VLBA) survey conducted as part of the DYNAMO-VLBA project, aimed at measuring the dynamical masses of young stellar…

astro-ph.SR2026

Dynamical masses of YSOs with the VLBA: DYNAMO VLBA: Trigonometric parallaxes and proper motions of YSOs in Orion

Sergio A. Dzib, Jazmín Ordóñez-Toro, Laurent Loinard +9

We present results from a multi-epoch Very Long Baseline Array (VLBA) survey of compact radio sources in the Orion complex, conducted within both the DYNAMO-VLBA and the GOBELINS p…

astro-ph.GA2026

Resolved Dust Emission and CO Isotopologues in Giant Molecular Clouds of the Andromeda Galaxy

Chloe Bosomworth, Jan Forbrich, Charles J. Lada +1

Dust emission at submillimeter wavelengths can be used to reliably trace the basic properties of molecular clouds. Early results from a recent Submillimeter Array (SMA) survey of t…

astro-ph.GA2025

Differential virial analysis: a new technique to determine the dynamical state of molecular clouds

Mark R. Krumholz, Charles J. Lada, Jan Forbrich

Since molecular clouds form stars, at least some parts of them must be in a state of collapse. However, there is a long-standing debate as to whether that collapse is local, involv…

astro-ph.GA2025

The SKA Galactic Centre Survey -- A White Paper

Rainer Schoedel, Antxon Alberdi, Izaskun Jimenez-Serra +17

With its extreme density of stars and stellar remnants, dense young massive clusters, high specific star formation rate, intense radiation field, high magnetic field strength, and…

astro-ph.SR2025

The past, present and future of observations of externally irradiated disks

Planet formation environments collaboration, Megan Allen, Rossella Anania +51

Recent years have seen a surge of interest in the community studying the effect of ultraviolet radiation environment, predominantly set by OB stars, on protoplanetary disc evolutio…