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20162026
most citedNew Constraints on the CO(2-1)/(1-0) Line Ratio Across Nearby Disc Galaxies

130 citations · 1.2k across the 41 of their papers we have counts for

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Showing 2019Show all

7 papers · 1 filter

astro-ph.GA2019

6.7 GHz CH3OH absorption towards the N3 Galactic Center point-source

Natalie Butterfield, Adam Ginsburg, Dominic Ludovici +4

We present evidence of 6.7 GHz methanol (CH3OH)~and 4.8 GHz formaldehyde (H2CO) absorption towards the Galactic Center (GC) point-source `N3'. Both absorption features are unresolv…

astro-ph.GA2019

A Census of Early Phase High-Mass Star Formation in the Central Molecular Zone

Xing Lu, Elisabeth A. C. Mills, Adam Ginsburg +13

We present new observations of C-band continuum emission and masers to assess high-mass (8 ) star formation at early evolutionary phases in the inner 200 pc of the Cent…

astro-ph.GA2019

Interstellar Plunging Waves: ALMA resolves the physical structure of non-stationary MHD shocks

Giuliana Cosentino, Izaskun Jiménez-Serra, Paola Caselli +6

Magneto-hydrodynamic (MHD) shocks are violent events that inject large amounts of energy in the interstellar medium (ISM) dramatically modifying its physical properties and chemica…

astro-ph.GA201941 cited

Young massive star cluster formation in the Galactic Centre is driven by global gravitational collapse of high-mass molecular clouds

A. T. Barnes, S. N. Longmore, A. Avison +19

Young massive clusters (YMCs) are the most compact, high-mass stellar systems still forming at the present day. The precursor clouds to such systems are, however, rare due to their…

astro-ph.GA2019107 cited

'The Brick' is not a brick: A comprehensive study of the structure and dynamics of the Central Molecular Zone cloud G0.253+0.016

J. D. Henshaw, A. Ginsburg, T. J. Haworth +19

In this paper we provide a comprehensive description of the internal dynamics of G0.253+0.016 (a.k.a. 'the Brick'); one of the most massive and dense molecular clouds in the Galaxy…

astro-ph.GA201991 cited

The dynamical evolution of molecular clouds near the Galactic Centre - II. Spatial structure and kinematics of simulated clouds

J. M. D. Kruijssen, J. E. Dale, S. N. Longmore +16

The evolution of molecular clouds in galactic centres is thought to differ from that in galactic discs due to a significant influence of the external gravitational potential. We pr…