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The curious morphology and orientation of Orion proplyd HST-10
Ralph Y. Shuping, Marc Kassis, John Bally +1
HST-10 is one of the largest proplyds in the Orion Nebula and is located approximately 1' SE of the Trapezium. Unlike other proplyds in Orion, however, the long-axis of HST-10 does…
The Bolocam Galactic Plane Survey. X. A Complete Spectroscopic Catalog of Dense Molecular Gas Observed toward 1.1 mm Dust Continuum Sources with 7.5 <= l <= 194 degrees
Yancy L. Shirley, Timothy P. Ellsworth-Bowers, Brian Svoboda +10
The Bolocam Galactic Plane Survey (BGPS) is a 1.1 mm continuum survey of dense clumps of dust throughout the Galaxy covering 170 square degrees. We present spectroscopic observatio…
The Bolocam Galactic Plane Survey IX: Data Release 2 and Outer Galaxy Extension
Adam Ginsburg, Jason Glenn, Erik Rosolowsky +9
We present a re-reduction and expansion of the Bolocam Galactic Plane Survey, first presented by Aguirre et al. (2011) and Rosolowsky et al. (2010). The BGPS is a 1.1 mm survey of…
The Bolocam Galactic Plane Survey. VIII. A Mid-Infrared Kinematic Distance Discrimination Method
Timothy P. Ellsworth-Bowers, Jason Glenn, Erik Rosolowsky +6
We present a new distance estimation method for dust-continuum-identified molecular cloud clumps. Recent (sub-)millimeter Galactic plane surveys have cataloged tens of thousands of…
What controls star formation in the central 500 pc of the Galaxy?
J. M. Diederik Kruijssen, Steven N. Longmore, Bruce G. Elmegreen +4
The star formation rate (SFR) in the Central Molecular Zone (CMZ, i.e. the central 500 pc) of the Milky Way is lower by a factor of >10 than expected for the substantial amount of…