activity
19962024
most citedResolution of Distance Ambiguities of Inner Galaxy Massive Star Formation Regions II

99 citations · 1.1k across the 52 of their papers we have counts for

collaborators

50 papers

astro-ph.SR2024

Radio Continuum and Water Maser Observations of the High-Mass Protostar IRAS 19035+0641 A

Tatiana M. Rodriguez, Emmanuel Momjian, Peter Hofner +2

We present Very Large Array (VLA) 1.3 cm continuum and 22.2 GHz HO maser observations of the high-mass protostellar object IRAS 19035+0641 A. Our observations unveil an elongat…

astro-ph.GA2023★ 3 cited

Excited Hydroxyl Outflow in the High-Mass Star-Forming Region G34.26+0.15

W. S. Tan, E. D. Araya, C. Rigg +4

G34.26+0.15 is a region of high-mass star formation that contains a broad range of young stellar objects in different stages of evolution, including a hot molecular core, hyper-com…

astro-ph.GA2023

Broadband VLA Spectral Line Survey of a Sample of Ionized Jet Candidates

E. Sanchez-Tovar, E. D. Araya, V. Rosero +2

The study of the interaction between ionized jets, molecular outflows and their environments is critical to understanding high-mass star formation, especially because jets and outf…

astro-ph.GA2023★ 3 cited

Searching for Molecular Jets from High-Mass Protostars

Tatiana M. Rodriguez, Peter Hofner, Isaac Edelman +2

We report Very Large Array (VLA) observations in the Q-band toward 10 ionized jet candidates to search for SiO emission, a well-known shocked gas tracer. We detected 7 mm continuum…

astro-ph.GA2022

A global view on star formation: The GLOSTAR Galactic plane survey. VI. Radio Source Catalog II: and , VLA B-configuration

S. A. Dzib, A. Y. Yang, J. S. Urquhart +20

As part of the GLOSTAR survey we have used the VLA in its B-configuration to observe the part of the Galactic plane between longitudes of 28d and 36d and latitudes from -1d to +1d…

astro-ph.GA2021

Discovery of a Highly Collimated Flow from the High-Mass Protostar ISOSS J23053+5953 SMM2

T. M., Rodríguez, P. Hofner +7

We present Very Large Array C, X, and Q-band continuum observations, as well as 1.3 mm continuum and CO(2-1) observations with the Submillimeter Array toward the high-mass protoste…