R
Rahul Shetty
Researcher at Heidelberg University
Publications - 29
Citations - 2429
Rahul Shetty is an academic researcher from Heidelberg University. The author has contributed to research in topics: Molecular cloud & Star formation. The author has an hindex of 23, co-authored 29 publications receiving 2342 citations. Previous affiliations of Rahul Shetty include Harvard University & University of Maryland, College Park.
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The effect of line-of-sight temperature variation and noise on dust continuum observations
TL;DR: In this paper, the authors investigate the effect of line-of-sight temperature variations and noise on two commonly used methods to determine dust properties from dust-continuum observations of dense cores.
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Modeling CO Emission: I. CO as a Column Density Tracer and the X-Factor in Molecular Clouds
TL;DR: In this article, the authors apply radiative transfer calculations to these MC models in order to investigate the properties of CO line emission, including its relationship to the total, H2, and CO column densities, as well as the "X factor," the ratio of H2 column density to CO intensity.
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The effect of noise on the dust temperature-spectral index correlation
TL;DR: In this article, the authors investigate how uncertainties in flux measurements affect the results from modified blackbody spectral energy distribution (SED) fits, and show that an inverse correlation between the dust temperature T and spectral index β naturally arises from least-squares fits due to the uncertainties, even for sources with a single T and β.
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The Mass-size Relation from Clouds to Cores. II. Solar Neighborhood Clouds
Jens Kauffmann,Jens Kauffmann,Thushara Pillai,Thushara Pillai,Rahul Shetty,Rahul Shetty,Philip C. Myers,Alyssa A. Goodman +7 more
TL;DR: In this paper, the authors measured the mass and size of cloud fragments in several molecular clouds continuously over a wide range of spatial scales (0.05 − 0.15 - 0.34).
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Global Modeling of Spur Formation in Spiral Galaxies
Rahul Shetty,Eve C. Ostriker +1 more
TL;DR: In this article, the formation of substructure in spiral galaxies using global MHD simulations, including gas self-gravity, was investigated, and it was shown that a sufficiently strong spiral potential is required to produce true spurs, consisting of interarm structures emerging from gas concentrations in the main spiral arms.