85 citations · 180 across the 5 of their papers we have counts for
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CMZoom III: Spectral Line Data Release
Daniel Callanan, Steven N. Longmore, Cara Battersby +21
We present an overview and data release of the spectral line component of the SMA Large Program, \textit{CMZoom}. \textit{CMZoom} observed CO(2-1), CO(2-1) and C$^{18…
A Brief Update on the CMZoom Survey
Cara Battersby, Eric Keto, Qizhou Zhang +16
The inner few hundred parsecs of the Milky Way, the Central Molecular Zone (CMZ), is our closest laboratory for understanding star formation in the extreme environments (hot, dense…
Temperature structures in Galactic Center clouds - Direct evidence for gas heating via turbulence
K. Immer, J. Kauffmann, T. Pillai +2
The Central Molecular Zone (CMZ) at the center of our Galaxy is the best template to study star formation processes under extreme conditions, similar to those in high-redshift gala…
Diversity of chemistry and excitation conditions in the high-mass star forming complex W33
K. Immer, R. Galván-Madrid, C. König +2
The object W33 is a giant molecular cloud that contains star forming regions at various evolutionary stages from quiescent clumps to developed H II regions. Since its star forming…
Trigonometric Parallaxes of Star Forming Regions in the Scutum Spiral Arm
M. Sato, Y. W. Wu, K. Immer +6
We report measurements of trigonometric parallaxes for six high-mass star-forming regions in the Scutum spiral arm of the Milky Way as part of the BeSSeL Survey. Combining our meas…