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Rahul Shetty

3 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author2

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA2
  • astro-ph.SR1
ORCID 0009-0009-6197-8110

identity via Semantic Scholar / OpenAlex

most citedUsing CO line ratios to trace the physical properties of molecular clouds

59 citations · 120 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2016★ 59 cited

Using CO line ratios to trace the physical properties of molecular clouds

Camilo H. Peñaloza, Paul C. Clark, Simon C. O. Glover +2

The carbon monoxide (CO) rotational transition lines are the most common tracers of molecular gas within giant molecular clouds (MCs). We study the ratio (R2−1/1−0​) between CO…

astro-ph.SR2014★ 19 cited

Centroid Velocity Statistics of Molecular Clouds

Erik Bertram, Lukas Konstandin, Rahul Shetty +2

We compute structure functions and Fourier spectra of 2D centroid velocity (CV) maps in order to study the gas dynamics of typical molecular clouds (MCs) in numerical simulations.…

astro-ph.GA2014★ 42 cited

Interpreting the sub-linear Kennicutt-Schmidt relationship: The case for diffuse molecular gas

Rahul Shetty, Paul C. Clark, Ralf S. Klessen

Recent statistical analysis of two extragalactic observational surveys strongly indicate a sublinear Kennicutt-Schmidt (KS) relationship between the star formation rate (Sigsfr) an…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.