activity
20102026
most citedWeak and Compact Radio Emission in Early High-Mass Star Forming Regions: I. VLA Observations

75 citations · 375 across the 29 of their papers we have counts for

collaborators

28 papers

astro-ph.SR2026

An Eccentric Massive Protobinary Assembled via a Core-merger Parabolic Encounter

Yao Wang, Yichen Zhang, Rubén Fedriani +14

Most massive stars form in binary systems, which profoundly influence their subsequent evolution. However, how such systems form remains poorly understood, with several competing s…

astro-ph.SR2026

Unveiling Ionized Jet Morphologies: Sub-arcsecond VLA Observations of Compact Radio Sources

Tatiana M. Rodriguez, Peter Hofner, Emmanuel Momjian +3

We present sub-arcsecond () resolution VLA 1.3 cm continuum and 22.2 GHz HO maser observations toward 15 compact radio continuum sources with rising sp…

astro-ph.SR2025

The SOFIA Massive (SOMA) Radio Survey. II. Radio Emission from High-Luminosity Protostars

Francisco Sequeira-Murillo, Viviana Rosero, Joshua Marvil +9

We present centimeter continuum observations of seven high luminosity massive protostars and their surrounding sources in regions with multiple targets, as part of the SOFIA Massiv…

astro-ph.SR2025★ 1 cited

The SOFIA Massive (SOMA) Star Formation Q-band Follow-up. II. Hydrogen Recombination Lines Toward High-Mass Protostars

Prasanta Gorai, Kotomi Taniguchi, Jonathan C. Tan +11

Hydrogen recombination lines (HRLs) are valuable diagnostics of the physical conditions in ionized regions around high-mass stars. Understanding their broadening mechanisms and int…

astro-ph.GA2024

The SOFIA Massive (SOMA) Star Formation Survey. V. Clustered Protostars

Zoie Telkamp, Ruben Fedriani, Jonathan C. Tan +16

We present m SOFIA-FORCAST images of seven regions of ``clustered" star formation as part of the SOFIA Massive (SOMA) Star Formation Survey. We identify a total of 34…

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…