collaborators

6 papers

astro-ph.SR2026

Orbital motion and dynamical mass of the complex periodic variable binary system 2MASS J05082729-2101444

S. Curiel, G. N. Ortiz-León, V. J. S. Béjar +22

We used very long baseline interferometry to constrain the orbit of the binary system 2MASS J05082729-2101444. We observed the system with the VLBA in three epochs at a frequency o…

astro-ph.GA2025

A global view on star formation: The GLOSTAR Galactic plane survey XII. Effelsberg's continuum view and data release

Y. Gong, W. Reich, M. R. Rugel +24

Extended radio continuum emission and its linear polarization play a key role in probing large-scale structures of synchrotron and free-free emission in the Milky Way. Despite the…

astro-ph.GA2025

Survey of (sub)mm water masers in low-mass star-forming regions

P. K. Humire, C. Goddi, G. N. Ortiz-León +2

Water masers are common in star-forming regions (SFRs), with the 22.235 GHz transition widely detected in both high- and low-mass protostars. In contrast, (sub)millimeter water mas…

astro-ph.SR2025

Dynamical mass of the Serpens intermediate-mass young stellar system EC\,95 with DYNAMO--VLBA

Jazmín Ordóñez-Toro, Sergio A. Dzib, Laurent Loinard +8

We present dynamical mass measurements, obtained from multi-epoch Very Long Baseline Interferometry (VLBI) observations, for the young multiple stellar system EC\,95, located in th…

astro-ph.SR2025

VLBA Detections in the Oph-S1 Binary System near Periastron Confirmation of its Orbital Elements and Mass

Jazmín Ordóñez-Toro, Sergio A. Dzib, Laurent Loinard +7

Oph-S1 is the most luminous and massive stellar member of the nearby Ophiuchus star-forming region. Previous Very Long Baseline Array (VLBA) observations have shown it to be an int…

astro-ph.HE2025

A multi-frequency study of sub-parsec jets with the Event Horizon Telescope

Jan Röder, Maciek Wielgus, Andrei P. Lobanov +287

The 2017 observing campaign of the Event Horizon Telescope (EHT) delivered the first very long baseline interferometry (VLBI) images at the observing frequency of 230 GHz, leading…