activity
20222026
most citedThe physical and chemical structure of Sagittarius B2 -- VI. UCHII regions in Sgr B2

21 citations · 31 across the 20 of their papers we have counts for

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Showing 2025Show all

7 papers · 1 filter

astro-ph.GA2025

The Colors of Ices: Measuring ice column density through photometry

Adam Ginsburg, Savannah R. Gramze, Matthew L. N. Ashby +8

Ices imprint strong absorption features in the near- and mid-infrared, but until recently they have been studied almost exclusively with spectroscopy toward small samples of bright…

astro-ph.GA2025

ALMA-IMF XX: Core fragmentation in the W51 high-mass star-forming region

T. Yoo, A. Ginsburg, J. Braine +27

We present a study of core fragmentation in the W51-E and W51-IRS2 protoclusters in the W51 high-mass star-forming region. The identification of core fragmentation is achieved by t…

astro-ph.GA2025

Mapping CO Ice in a Star-Forming Filament in the 3 kpc Arm with JWST

Savannah Gramze, Adam Ginsburg, Nazar Budaiev +14

CO gas emission is a fundamental tool for measuring column density, but in cold, dark clouds, much of the CO is locked away in ice. We present JWST results from observations of a s…

astro-ph.GA2025

JWST's first view of the most vigorously star-forming cloud in the Galactic center -- Sagittarius B2

Nazar Budaiev, Adam Ginsburg, Ashley T. Barnes +9

We report JWST NIRCAM and MIRI observations of Sgr B2, one of the most active sites of star formation in the Galaxy. These observations, using 14 filters spanning 1.5 to 25 microns…

astro-ph.GA2025

Properties of masers and their associated sources in Sagittarius B2

Nazar Budaiev, Adam Ginsburg, Ciriaco Goddi +5

We present high-resolution Karl G. Jansky Very Large Array observations of the 22 GHz maser line in the extended Sagittarius B2 cloud. We detect 499 …

astro-ph.GA2025★ 6 cited

Dual-band Unified Exploration of Three CMZ Clouds (DUET). Cloud-wide census of continuum sources showing low spectral indices

Fengwei Xu, Xing Lu, Ke Wang +19

The Milky Way's Central Molecular Zone (CMZ) is measured to form stars 10 times less efficiently than in the Galactic disk, based on emission from high-mass stars. However, the CMZ…

astro-ph.GA2025

Subclustering and Star Formation Efficiency in Three Protoclusters in the Central Molecular Zone

Suinan Zhang, Xing Lu, Adam Ginsburg +21

We present so far the highest resolution (0.04") ALMA 1.3 mm continuum observations of three massive star-forming clumps in the Central Molecular Zone, namely 20 km s…