activity
20122026
most citedThe WISE Catalog of Galactic HII Regions

414 citations · 1.1k across the 41 of their papers we have counts for

collaborators

39 papers

astro-ph.GA2026

Metallicity Structure in Galactic Longitude-Velocity Diagrams of the Milky Way Disk and FIRE-2 Simulations

Victor Liu, Dana S. Balser, Trey V. Wenger

We investigate longitude-velocity (-) diagrams as a diagnostic tool to study the metallicity structure of the Milky Way (MW) disk. The present-day metallicity structure en…

astro-ph.GA2025★ 7 cited

Bar-spiral interaction produces radial migration and star formation bursts

Léa Marques, Ivan Minchev, Bridget Ratcliffe +8

Central bars and spirals are known to strongly impact the evolution of their host galaxies, both in terms of dynamics and star formation. Their typically different pattern speeds c…

astro-ph.IM2024

$\texttt{bayes_spec}$: A Bayesian Spectral Line Modeling Framework for Astrophysics

Trey V. Wenger

$\texttt{bayes_spec}$ is a Bayesian spectral line modeling framework for astrophysics. Given a user-defined model and a spectral line dataset, $\texttt{bayes_spec}$ enables inferen…

astro-ph.GA2024

Revisiting the Vertical Distribution of HI Absorbing Clouds in the Solar Neighborhood. II. Constraints from a Large Catalog of 21 cm Absorption Observations at High Galactic Latitudes

Daniel R. Rybarczyk, Trey V. Wenger, Snezana Stanimirović

The cold neutral medium (CNM) is where neutral atomic hydrogen (HI) is converted into molecular clouds, so the structure and kinematics of the CNM are key drivers of galaxy evoluti…

astro-ph.GA2024

The Most Sensitive Radio Recombination Line Measurements Ever Made of the Galactic Warm Ionized Medium

T. M. Bania, Dana S. Balser, Trey V. Wenger +3

Diffuse ionized gas pervades the disk of the Milky Way. We detect extremely faint emission from this Galactic Warm Ionized Medium (WIM) using the Green Bank Telescope to make radio…

astro-ph.GA2024

Revisiting the Vertical Distribution of HI Absorbing Clouds in the Solar Neighborhood

Trey V. Wenger, Daniel R. Rybarczyk, Snežana Stanimirović

The vertical distribution of cold neutral hydrogen (HI) clouds is a constraint on models of the structure, dynamics, and hydrostatic balance of the interstellar medium. In 1978, Cr…

astro-ph.GA2024

The Metallicity-Electron Temperature Relationship in HII Regions

Dana S. Balser, Trey V. Wenger

HII region heavy-element abundances throughout the Galactic disk provide important constraints to theories of the formation and evolution of the Milky Way. In LTE, radio recombinat…

astro-ph.IM2023

Methods for Averaging Spectral Line Data

L. D. Anderson, B. Liu, Dana S. Balser +5

The ideal spectral averaging method depends on one's science goals and the available information about one's data. Including low-quality data in the average can decrease the signal…

astro-ph.GA2023

The GBT Diffuse Ionized Gas Survey (GDIGS): Discrete Sources

Dylan J. Linville, Matteo Luisi, L. D. Anderson +6

The Green Bank Telescope (GBT) Diffuse Ionized Gas Survey (GDIGS) traces ionized gas in the Galactic midplane by observing radio recombination line (RRL) emission from 4-8 GHz. The…

astro-ph.GA2023★ 13 cited

A comparison of the Milky Way's recent star formation revealed by dust thermal emission and high-mass stars

J. D. Soler, E. Zari, D. Elia +10

We present a comparison of the Milky Way's star formation rate (SFR) surface density () obtained with two independent state-of-the-art observational methods. The first…

astro-ph.SR2022★ 6 cited

Do All Low-Mass Stars Undergo Extra Mixing Processes?

Dana S. Balser, Trey V. Wenger, T. M. Bania

Standard stellar evolution models that only consider convection as a physical process to mix material inside of stars predict the production of significant amounts of 3He in low-ma…

astro-ph.GA2021★ 4 cited

Discovery of a New Population of Galactic HII Regions with Ionized Gas Velocity Gradients

Dana S. Balser, Trey V. Wenger, L. D. Anderson +4

We investigate the kinematic properties of Galactic HII regions using radio recombination line (RRL) emission detected by the Australia Telescope Compact Array (ATCA) at 4-10 GHz a…

astro-ph.GA2021★ 20 cited

The Southern HII Region Discovery Survey. II. The Full Catalog

Trey V. Wenger, J. R. Dawson, John M. Dickey +6

The Southern HII Region Discovery Survey (SHRDS) is a 900 hour Australia Telescope Compact Array 4-10 GHz radio continuum and radio recombination line (RRL) survey of Galactic HII…

astro-ph.GA2021★ 26 cited

The GBT Diffuse Ionized Gas Survey (GDIGS): Survey Overview and First Data Release

L. D. Anderson, Matteo Luisi, Bin Liu +6

The Green Bank Telescope (GBT) Diffuse Ionized Gas Survey (GDIGS) traces ionized gas in the Galactic midplane by measuring GHz radio recombination line (RRL) emission. The nom…

astro-ph.GA2021

A VLA Census of the Galactic H II Region Population

William P. Armentrout, Loren D. Anderson, Trey V. Wenger +2

The Milky Way contains thousands of H II region candidates identified by their characteristic mid-infrared morphology, but lacking detections of ionized gas tracers such as radio c…

astro-ph.GA2021★ 10 cited

The Galactic HII Region Luminosity Function at Radio and Infrared Wavelengths

J. L. Mascoop, L. D. Anderson, Trey. V. Wenger +4

The Galactic HII region luminosity function (LF) is an important metric for understanding global star formation properties of the Milky Way, but only a few studies have been done a…

astro-ph.GA2019★ 12 cited

The GBT Diffuse Ionized Gas Survey: Tracing the Diffuse Ionized Gas around the Giant HII Region W43

Matteo Luisi, L. D. Anderson, Bin Liu +4

The Green Bank Telescope (GBT) Diffuse Ionized Gas Survey (GDIGS) is a fully-sampled radio recombination line (RRL) survey of the inner Galaxy at C-band (4-8 GHz). We average toget…

astro-ph.GA2019★ 70 cited

Metallicity Structure in the Milky Way Disk Revealed by Galactic HII Regions

Trey V. Wenger, Dana S. Balser, L. D. Anderson +1

The metallicity structure of the Milky Way disk stems from the chemodynamical evolutionary history of the Galaxy. We use the National Radio Astronomy Observatory Karl G. Jansky Ver…

astro-ph.GA2019

Canadian Investigations of the Interstellar Medium

Alex S. Hill, Jan Cami, Laura Fissel +10

The interstellar medium mediates galactic evolution as the reservoir of material for future star formation and the repository of energy and matter output by stellar processes. Cana…

astro-ph.GA2019★ 7 cited

The Occurrence of Compact Groups of Galaxies Through Cosmic Time

Christopher D. Wiens, Trey V. Wenger, Panayiotis Tzanavaris +3

We use the outputs of a semi-analytical model of galaxy formation run on the Millennium Simulation to investigate the prevalence of 3D compact groups (CGs) of galaxies from $z = 11…

astro-ph.GA2018★ 23 cited

The Southern HII Region Discovery Survey I: The Bright Catalog

Trey V. Wenger, John. M. Dickey, C. H. Jordan +7

The census of Galactic HII regions is vastly incomplete in the Southern sky. We use the Australia Telescope Compact Array (ATCA) to observe 4-10 GHz radio continuum and hydrogen ra…

astro-ph.GA2018★ 36 cited

A Galactic Plane Defined by the Milky Way HII Region Distribution

L. D. Anderson, Trey V. Wenger, W. P. Armentrout +2

We develop a framework for a new definition of the Galactic midplane, allowing for tilt (rotation about Galactic azimuth 90deg.), and roll (rotation about Galactic azimuth 0deg.) o…

astro-ph.GA2018★ 13 cited

Astrochemical Kinetic Grid Models of Groups of Observed Molecular Abundances: Taurus Molecular Cloud 1 (TMC-1)

Dominique M. Maffucci, Trey V. Wenger, Romane Le Gal +1

The emission line spectra of cyanoacetylene and methanol reveal chemical and physical heterogeneity on very small (< 0.1 pc) scales toward the peak in cyanopolyyne emission in the…

astro-ph.GA2018★ 1 cited

Science with an ngVLA: Radio Recombination Lines from HII Regions

Dana S. Balser, L. D. Anderson, T. M. Bania +4

The ngVLA will create a Galaxy-wide, volume-limited sample of HII regions; solve some long standing problems in the physics of HII regions; and provide an extinction-free star form…