activity
20072016
most citedMaximally Star-Forming Galactic Disks I. Starburst Regulation Via Feedback-Driven Turbulence

344 citations · 2.9k across the 33 of their papers we have counts for

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Showing 2013Show all

6 papers · 1 filter

astro-ph.GA2013★ 113 cited

Quantifying Observational Projection Effects Using Molecular Cloud Simulations

Christopher N. Beaumont, Stella S. R. Offner, Rahul Shetty +2

The physical properties of molecular clouds are often measured using spectral-line observations, which provide the only probes of the clouds' velocity structure. It is hard, though…

astro-ph.SR2013★ 11 cited

Hierarchical Bayesian analysis of the velocity power spectrum in supersonic turbulence

Lukas Konstandin, Rahul Shetty, Philipp Girichidis +1

Turbulence is a dominant feature operating in gaseous flows across nearly all scales in astrophysical environments. Accordingly, accurately estimating the statistical properties of…

astro-ph.SR2013★ 1 cited

Relationship between molecular cloud structure and density PDFs

Orlin Stanchev, Sava Donkov, Todor V. Veltchev +1

Volume and column density PDFs in molecular clouds are important diagnostics for understanding their general structure. We developed a novel approach to trace the cloud structure b…

astro-ph.CO2013★ 51 cited

Indications of a sub-linear and non-universal Kennicutt-Schmidt relationship

Rahul Shetty, Brandon C. Kelly, Nurur Rahman +5

We estimate the parameters of the Kennicutt-Schmidt (KS) relationship, linking the star formation rate (Sigma_SFR) to the molecular gas surface density (Sigma_mol), in the STING sa…

astro-ph.GA2013★ 62 cited

Line Profiles of Cores within Clusters: II Signatures of Dynamical Collapse during High Mass Star Formation

Rowan J. Smith, Rahul Shetty, Henrik Beuther +2

Observations of atomic or molecular lines can provide important information about the physical state of star forming regions. In order to investigate the line profiles from dynamic…

astro-ph.GA2013★ 64 cited

On the temperature structure of the Galactic Centre cloud G0.253+0.016

Paul C Clark, Simon C. O. Glover, Sarah E. Ragan +2

We present a series of smoothed particle hydrodynamical models of G0.253+0.016 (also known as 'The Brick'), a very dense molecular cloud that lies close to the Galactic Centre. We…