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The Bolocam Galactic Plane Survey. XIV. Physical Properties of Massive Starless and Star Forming Clumps
Brian E Svoboda, Yancy L Shirley, Cara Battersby +8
We sort molecular clouds between from the Bolocam Galactic Plane Survey based on observational diagnostics of star formation activity: compact $70…
Large-scale latitude distortions of the inner Milky Way Disk from the Herschel/Hi-GAL Survey
Sergio Molinari, Alberto Noriega-Crespo, John Bally +9
We use the Herschel Hi-GAL survey data to study the spatial distribution in Galactic longitude and latitude of the interstellar medium and of dense, star-forming clumps in the inne…
Dense gas in the Galactic central molecular zone is warm and heated by turbulence
Adam Ginsburg, Christian Henkel, Yiping Ao +19
The Galactic center is the closest region in which we can study star formation under extreme physical conditions like those in high-redshift galaxies. We measure the temperature of…
ALMA Observations of the Largest Proto-Planetary Disk in the Orion Nebula, 114-426: A CO Silhouette
John Bally, Rita K. Mann, Josh Eisner +7
We present ALMA observations of the largest protoplanetary disk in the Orion Nebula, 114-426. Detectable 345 GHz (856 micron) dust continuum is produced only in the 350 AU central…
Nested shells reveal the rejuvenation of the Orion-Eridanus superbubble
B. B. Ochsendorf, A. G. A. Brown, J. Bally +1
The Orion-Eridanus superbubble is the prototypical superbubble due to its proximity and evolutionary state. Here, we provide a synthesis of recent observational data from WISE and…
The Bolocam Galactic Plane Survey. XIII. Physical Properties and Mass Functions of Dense Molecular Cloud Structures
Timothy P. Ellsworth-Bowers, Jason Glenn, Allyssa Riley +7
We use the distance probability density function (DPDF) formalism of Ellsworth-Bowers et al. (2013, 2015) to derive physical properties for the collection of 1,710 Bolocam Galactic…
The Orion Fingers: Near-IR Adaptive Optics Imaging of an Explosive Protostellar Outflow
John Bally, Adam Ginsburg, Devin Silvia +1
Aims. Adaptive optics images are used to test the hypothesis that the explosive BN/KL outflow from the Orion OMC1 cloud core was powered by the dynamical decay of a non-hierarchica…
The Bolocam Galactic Plane Survey. XI. Temperatures and Substructure of Galactic Clumps Based on 350 micron Observations
Manuel Merello, Neal J. Evans, Yancy L. Shirley +5
We present 107 maps of continuum emission at 350 microns from Galactic molecular clumps. Observed sources were mainly selected from the Bolocam Galactic Plane Survey (BGPS) catalog…