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20132026
most citedThe Bolocam Galactic Plane Survey. XIV. Physical Properties of Massive Starless and Star Forming Clumps

103 citations · 835 across the 22 of their papers we have counts for

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17 papers · 1 filter

astro-ph.GA2026

Deuteration of Organic Molecules as a Probe of Starless Core and Filament Evolution in Barnard 10

Hanga Andras-Letanovszky, Yancy L. Shirley, Lucille J. Steffes +4

The deuterium fractionation of molecules in starless cores is sensitive to their dynamical histories, which recent magnetohydrodynamical simulations have shown to be extremely vari…

astro-ph.GA2023

CMZoom IV. Incipient High-Mass Star Formation Throughout the Central Molecular Zone

H Perry Hatchfield, Cara Battersby, Ashley T. Barnes +15

In this work, we constrain the star-forming properties of all possible sites of incipient high-mass star formation in the Milky Way's Galactic Center. We identify dense structures…

astro-ph.GA2023★ 14 cited

Evidence of a Cloud-Cloud Collision from Overshooting Gas in the Galactic Center

Savannah R. Gramze, Adam Ginsburg, David S. Meier +4

The Milky Way is a barred spiral galaxy with "bar lanes" that bring gas towards the Galactic Center. Gas flowing along these bar lanes often overshoots, and instead of accreting on…

astro-ph.GA2023★ 11 cited

3D Radiative Transfer Modelling and Virial Analysis of Starless Cores in the B10 Region of the Taurus Molecular Cloud

Samantha Scibelli, Yancy Shirley, Anika Schmiedeke +4

Low-mass stars like our Sun begin their evolution within cold (10 K) and dense ( cm) cores of gas and dust. The physical structure of starless cores is best probe…

astro-ph.GA2022★ 14 cited

FAUST VI. VLA 1623--2417 B: a new laboratory for astrochemistry around protostars on 50 au scale

C. Codella, A. López-Sepulcre, S. Ohashi +25

The ALMA interferometer, with its unprecedented combination of high-sensitivity and high-angular resolution, allows for (sub-)mm wavelength mapping of protostellar systems at Solar…

astro-ph.GA2022★ 22 cited

Hot methanol in the [BHB2007] 11 protobinary system: hot corino versus shock origin? : FAUST V

C. Vastel, F. Alves, C. Ceccarelli +63

Methanol is a ubiquitous species commonly found in the molecular interstellar medium. It is also a crucial seed species for the building-up of the chemical complexity in star formi…

astro-ph.GA2022★ 32 cited

FAUST III. Misaligned rotations of the envelope, outflow, and disks in the multiple protostellar system of VLA 16232417

Satoshi Ohashi, Claudio Codella, Nami Sakai +69

We report a study of the low-mass Class-0 multiple system VLA 1623AB in the Ophiuchus star-forming region, using HCO (), CS (), and CCH () lines as…

astro-ph.GA2021★ 95 cited

ALMA-IMF I -- Investigating the origin of stellar masses: Introduction to the Large Program and first results

F. Motte, S. Bontemps, T. Csengeri +61

The ALMA-IMF Large Program imaged a total noncontiguous area of 53pc2, covering 15 extreme, nearby protoclusters of the Milky Way. They were selected to span relevant early protocl…

astro-ph.GA2021★ 39 cited

ALMA-IMF II -- investigating the origin of stellar masses: Continuum Images and Data Processing

A. Ginsburg, T. Csengeri, R. Galván-Madrid +49

We present the first data release of the ALMA-IMF Large Program, which covers the 12m-array continuum calibration and imaging. The ALMA-IMF Large Program is a survey of fifteen den…

astro-ph.GA2020★ 23 cited

The MUSTANG-2 Galactic Plane Survey (MGPS90) pilot

Adam Ginsburg, L. D. Anderson, Simon Dicker +19

We report the results of a pilot program for a Green Bank Telescope (GBT) MUSTANG Galactic Plane survey at 3 mm (90 GHz), MGPS90. The survey achieves a typical depth of …

astro-ph.GA2019★ 70 cited

ALMA observations of fragmentation, sub-structure, and protostars in high-mass starless clump candidates

Brian E. Svoboda, Yancy L. Shirley, Alessio Traficante +7

(Abridged) The initial physical conditions of high-mass stars and protoclusters remain poorly characterized. To this end we present the first targeted ALMA 1.3mm continuum and spec…

astro-ph.GA2018★ 15 cited

Searching for Inflow Towards Massive Starless Clump Candidates Identified in the Bolocam Galactic Plane Survey

Jenny Calahan, Yancy Shirley, Brian Svoboda +22

Recent Galactic plane surveys of dust continuum emission at long wavelengths have identified a population of dense, massive clumps with no evidence for on-going star formation. The…

astro-ph.GA2017★ 31 cited

The Lifetimes of Phases in High-Mass Star-Forming Regions

Cara Battersby, John Bally, Brian Svoboda

High-mass stars form within star clusters from dense, molecular regions, but is the process of cluster formation slow and hydrostatic or quick and dynamic? We link the physical pro…

astro-ph.GA2015★ 103 cited

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…

astro-ph.GA2014★ 49 cited

The Bolocam Galactic Plane Survey. XII. Distance Catalog Expansion Using Kinematic Isolation of Dense Molecular Cloud Structures With 13CO(1-0)

Timothy P. Ellsworth-Bowers, Erik Rosolowsky, Jason Glenn +5

We present an expanded distance catalog for 1,710 molecular cloud structures identified in the Bolocam Galactic Plane Survey (BGPS) version 2, representing a nearly threefold incre…

astro-ph.GA2013★ 53 cited

Ammonia Thermometry of Star Forming Galaxies

Jeffrey G. Mangum, Jeremy Darling, Christian Henkel +4

With a goal toward deriving the physical conditions in external galaxies, we present a study of the ammonia (NH) emission and absorption in a sample of star forming systems. Us…

astro-ph.GA2013★ 65 cited

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…