activity
20132026
most citedNext Generation Very Large Array Memo No. 5: Science Working Groups -- Project Overview

24 citations · 48 across the 9 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2026

JWST Observations of Starbursts: A Young Bubble in NGC 253's Central Starburst

Kaitlyn E. Sheriff, Elisabeth A. C. Mills, Xinyu Mai +31

We present a multi-wavelength analysis of a young bubble in the nuclear starburst of NGC 253 using new JWST MIRI-MRS observations together with archival ALMA (100, 350, 690 GHz) an…

astro-ph.GA2026

Reconciling 3D Models for the Central 10 parsecs of the Milky Way

Elisabeth A. C. Mills, Natalie O. Butterfield, Hauyu Baobab Liu +13

The construction of an accurate 3D model of the Milky Way center is necessary to understand inflow processes that drive its overall evolution, and to compare our Galactic nucleus t…

astro-ph.GA2026

ALMA Central Molecular Zone Exploration Survey (ACES) I: Overview

Steven N. Longmore, John Bally, Ashley T. Barnes +95

The mass flows and energy cycles within the inner regions of galaxies exert a powerful influence on the evolution of the galaxy population. The centre of the Milky Way is the only…

astro-ph.GA2025

Nonthermal Pressures: Key to Energy Balance and Structure Formation Near Sgr A* in the Milky Way

Farideh Mazoochi, Fatemeh S. Tabatabaei, Ashley T. Barnes +14

The circumnuclear region of the Galactic Center offers a unique laboratory to study energy balance and structure formation around Sgr A. This work investigates thermal and n…

astro-ph.GA2025★ 5 cited

JWST Observations of Starbursts: PAHs Closely Trace the Cool Phase of M82's Galactic Wind

Sebastian Lopez, Colton Ring, Adam K. Leroy +30

Stellar feedback drives multiphase gas outflows from starburst galaxies, but the interpretation of dust emission in these winds remains uncertain. To investigate this, we analyze n…

astro-ph.HE2025

Serendipitous discovery of a young cluster of galaxies at projected next to the nearby tadpole galaxy KUG 1138 + 327

Q. Daniel Wang, Juergen Ott

Using a 90 ks Chandra ACIS-S observation in the 0.3--7 keV band, along with complementary Low-Frequency Array and Karl G.~Jansky Very Large Array data in the 120--168 MHz and 1--2…

astro-ph.GA2023★ 1 cited

Where do stars explode in the ISM? -- The distribution of dense gas around evolved massive stars in M33

Sumit K. Sarbadhicary, Jordan Wagner, Eric W. Koch +27

The effect of supernovae (SNe) on star-formation in the interstellar medium (ISM) depends sensitively on where SNe explode with respect to ISM clouds. Observationally, SN ISM envir…

astro-ph.GA2021★ 14 cited

A wind-blown bubble in the Central Molecular Zone cloud G0.253+0.016

J. D. Henshaw, M. R. Krumholz, N. O. Butterfield +16

G0.253+0.016, commonly referred to as "the Brick" and located within the Central Molecular Zone, is one of the densest ( cm) molecular clouds in the Galaxy…

astro-ph.IM2015★ 24 cited

Next Generation Very Large Array Memo No. 5: Science Working Groups -- Project Overview

C. L. Carilli, M. McKinnon, J. Ott +17

We summarize the design, capabilities, and some of the priority science goals of a next generation Very Large Array (ngVLA). The ngVLA is an interferometric array with 10x larger e…

astro-ph.GA2013★ 4 cited

A Radio Survey of Galactic Center Clouds

E. A. C. Mills, C. C. Lang, M. R. Morris +5

We present a survey of molecules in a sample of Galactic center molecular clouds using the Karl G. Jansky Very large Array, which includes M0.25+0.01, the clouds near Sgr A, and Sg…