The 3D CMZ project builds a top-down view of our Galaxy's Center.
Recent Publications
- Circum-nuclear eccentric gas flow in the Galactic Center revealed by
ALMA CMZ Exploration Survey (ACES) June 13, 2025We analyze the CS (J=2-1) line cube from the internal data release obtained by the large-scale program "ALMA CMZ Exploration Survey (ACES)" to investigate the kinematic structure of the innermost $\sim 10$ pc region of the Galaxy, which contains the high-velocity compact cloud (HVCC) at $(l,b,v_{\rm lsr})\sim(+0^\circ.02,-0^\circ.02, 100 {\rm km~s}^{-1})$ (hereafter G0.02). The longitude-velocity diagram […]Yoshiaki Sofue
- ALMAGAL IV. Morphological comparison of molecular and thermal dust
emission using the histogram of oriented gradients (HOG) method April 17, 2025The study of molecular line emission is crucial to unveil the kinematics and the physical conditions of gas in star-forming regions. Our aim is to quantify the reliability of using individual molecular transitions to derive physical properties of the bulk of the H2 gas, looking at morphological correlations in their overall integrated molecular line emission […]C. Mininni
- The Galactic-Centre Arms inferred from ACES (ALMA CMZ Exploration
Survey) April 4, 2025Analyzing longitude-velocity diagrams (LVDs) in the CS(J=2-1) and H13CN(J=1-0) molecular lines from the internal release data of the ALMA Central-Molecular-Zone Exploration Survey (ACES) and in the 13CO (J=1-0) line from the Nobeyama Galactic-Centre (GC) survey, we identify six GC Arms as prominent straight LV ridges. In addition to the currently known Arms I to IV, […]Y. Sofue
- Dual-band Unified Exploration of Three CMZ Clouds (DUET). Cloud-wide
census of continuum sources showing low spectral indices March 31, 2025The 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's low-mass protostellar population, which accounts for most of the initial stellar mass budget and star formation rate (SFR), is poorly constrained observationally due to limited […]Fengwei Xu
- Discovery of a Giant Molecular Cloud at the Midpoint of the Galactic Bar
Dust Lanes: M4.7-0.8 March 18, 2025We present the detection of a previously unknown giant molecular cloud (GMC) located at the midpoint of the Galactic Bar Dust Lanes (M4.7--0.8), using spectral line observations taken with the Green Bank Telescope (GBT). This $\sim$60 pc long GMC is associated with accreting material that is transitioning from the quieter Galactic disk environment to the […]Natalie Butterfield
- ALMAGAL III. Compact source catalog: Fragmentation statistics and
physical evolution of the core population March 7, 2025The mechanisms behind the fragmentation of high-mass dense clumps into compact star-forming cores are fundamental topics in current astrophysical research. The ALMAGAL survey provides the opportunity to study this process at an unprecedented level of detail and statistical significance, featuring high-angular resolution $1.38$ mm ALMA observations of $1013$ massive dense clumps at various Galactic locations. […]A. Coletta
- ALMAGAL II. The ALMA evolutionary study of high-mass protocluster
formation in the Galaxy. ALMA data processing and pipeline March 7, 2025The ALMAGAL Large Program has observed 1017 high-mass star-forming regions distributed throughout the Galaxy, sampling different evolutionary stages and environmental conditions. In this work, we present the acquisition and processing of the ALMAGAL data. The main goal is to set up a robust pipeline that generates science-ready products, with a good and uniform quality across […]Á. Sánchez-Monge
- ALMAGAL I. The ALMA evolutionary study of high-mass protocluster
formation in the Galaxy. Presentation of the survey and early results March 7, 2025Fundamental questions about the physics responsible for fragmenting molecular parsec-scale clumps into cores of ~1000 au are still open, that only a statistically significant investigation with ALMA is able to address: what are the dominant agents that determine the core demographics, mass, and spatial distribution as a function of the physical properties of the hosting […]S. Molinari
News
3D CMZ Papers Make a SplashThe Milky Way Lab’s 3D CMZ project is now published and making a splash! The four papers: Battersby et al. 2025a: 3D CMZ. I. Central Molecular Zone Overview Battersby et al. 2025b: 3D CMZ. II. Hierarchical Structure Analysis of the Central Molecular Zone Walker et al. 2025: 3D CMZ. III. Constraining the 3D Structure of […]
MW Lab Press Conference at the AAS January 2025A press conference at the 245th meeting of the AAS on January 14th, 2025 presented by Danya Alboslani, a post-baccalaureate researcher working in the Milky Way Laboratory with Prof. Battersby. X-ray Echoes Reveal the 3D Structure of Molecular Clouds in our Galaxy’s Center A creative new method uses decades of data to learn about the […]
- The Milky Way Laboratory on the World Wide TelescopeLearn about the ground-breaking work the Milky Way Laboratory and its collaborators are doing through this World Wide Telescope tour! World Wide Telescope is a free and open-source platform showcasing a breadth of astronomical images for the public to enjoy and planetarium-like views of our night sky! First publicly demonstrated in 2008, the World Wide […]
The MW Lab at an Art Exhibit at the University of HartfordThe Milky Way Laboratory was invited to collaborate with Genevieve de Leon, the 2022-23 Koopman Distinguished Chair in the Painting Department at the University of Hartford, for an exhibition focused on the intersection between the Maya calendrical cycles and scientific studies of the cosmos. From the Milky Way Laboratory, H Perry Hatchfield, Jennifer Wallace, Dani […]
SgrE paper published!Graduate student Jennifer Wallace’s paper on molecular filaments observed towards the Sagittarius E star forming region has been published in ApJ! Congratulations, Jen! The Sgr E region is located near the dynamic intersection between the Galaxy’s Central Molecular Zone (CMZ) and the ‘far dust lane’, a stream of inflowing gas that helps transport material from the […]
Large collaborative ACES grant funded!Our collaborative NSF proposal (led by Prof. Betsy Mills at KU and co-PIed with Adam Ginsburg at UF, Qizhou Zhang at SAO, and John Bally at Colorado) to fund research studying gas flows in our Galaxy’s Center using the ACES survey (more below!) has been awarded! With the ALMA CMZ Exploration Survey, an approved ALMA […]
Meet the Milky Way Laboratory’s New Unofficial MascotWhile pursuing her research project to map out and analyze the minimum spanning trees (MSTs) of clouds in the Galactic Center using CMZoom Data, MW Lab undergraduate student Stefania Schuler, supervised by Jen Wallace, made an intriguing discovery. G0.316-0.201 is the designation of an isolated high-mass star-forming region in the CMZoom survey and it is […]