359 citations · 1.5k across the 40 of their papers we have counts for
12 papers · 1 filter
Complex investigations of an active star-formation region in southern part of Mon R2
T. A. Movsessian, J. Bally, T. Yu. Magakian +1
We continue to present the results of a Byurakan Narrow Band Imaging Survey (BNBIS). In this work we present the results of the search and further detailed investigation of the obj…
The JWST-NIRCam View of Sagittarius C. II. Evidence for Magnetically Dominated HII Regions in the CMZ
John Bally, Samuel Crowe, Rubén Fedriani +11
We present JWST-NIRCam narrow-band, 4.05 m Brackett- images of the Sgr C HII region, located in the Central Molecular Zone (CMZ) of the Galaxy. Unlike any HII region in the S…
3-D CMZ II: Hierarchical Structure Analysis of the Central Molecular Zone
Cara Battersby, Daniel L. Walker, Ashley Barnes +16
The Central Molecular Zone (CMZ) is the way station at the heart of our Milky Way Galaxy, connecting gas flowing in from Galactic scales with the central nucleus. Key open question…
3-D CMZ III: Constraining the 3-D structure of the Central Molecular Zone via molecular line emission and absorption
Daniel L. Walker, Cara Battersby, Dani Lipman +15
The Milky Way's Central Molecular Zone (CMZ) is the largest concentration of dense molecular gas in the Galaxy, the structure of which is shaped by the complex interplay between Ga…
The JWST-NIRCam View of Sagittarius C. I. Massive Star Formation and Protostellar Outflows
Samuel Crowe, Rubén Fedriani, Jonathan C. Tan +14
We present James Webb Space Telescope (JWST)-NIRCam observations of the massive star-forming molecular cloud Sagittarius C (Sgr C) in the Central Molecular Zone (CMZ). In conjuncti…
3-D CMZ I: Central Molecular Zone Overview
Cara Battersby, Daniel L. Walker, Ashley Barnes +16
The Central Molecular Zone (CMZ) is the largest reservoir of dense molecular gas in the Galaxy and is heavily obscured in the optical and near-IR. We present an overview of the far…
3-D CMZ IV: Distinguishing Near vs. Far Distances in the Galactic Center Using Spitzer and Herschel
Dani Lipman, Cara Battersby, Daniel L. Walker +15
A comprehensive 3-D model of the central 300 pc of the Milky Way, the Central Molecular Zone (CMZ) is of fundamental importance in understanding energy cycles in galactic nuclei, s…
Dynamical Accretion Flows -- ALMAGAL: Flows along filamentary structures in high-mass star-forming clusters
M. R. A. Wells, H. Beuther, S. Molinari +47
We use data from the ALMA Evolutionary Study of High Mass Protocluster Formation in the Galaxy (ALMAGAL) survey to study 100 ALMAGAL regions at 1 arsecond resolution located…
Accretion and Outflow in Orion-KL Source I
Melvyn Wright, Brett A. McGuire, Adam Ginsburg +6
We present ALMA observations of SiO, SiS, HO , NaCl, and SO line emission at ~30 to 50 mas resolution. These images map the molecular outflow and disk of Orion Source I (SrcI)…
SOFIA/FORCAST Galactic Center Source Catalog
Angela S. Cotera, Matthew J. Hankins, John Bally +12
The central regions of the Milky Way constitute a unique laboratory for a wide swath of astrophysical studies, consequently the inner 400 pc has been the target of numerous l…
Confirming the Explosive Dispersal Outflow in DR21 with ALMA
E. Guzmán Ccolque, M. Fernández López, L. A. Zapata +2
We present Atacama Large Millimeter/submillimeter Array (ALMA) 1.3 mm continuum and CO(2-1) line emission observations toward the high-mass star formation region DR21. Five new con…
The TEMPO Survey II: Science Cases Leveraged from a Proposed 30-Day Time Domain Survey of the Orion Nebula with the Nancy Grace Roman Space Telescope
Melinda Soares-Furtado, Mary Anne Limbach, Andrew Vanderburg +26
The TEMPO (Transiting Exosatellites, Moons, and Planets in Orion) Survey is a proposed 30-day observational campaign using the Nancy Grace Roman Space Telescope. By providing deep,…