Rahul Shetty, Ph.D.
Affiliations: | 2007 | Astronomy | University of Maryland, College Park, College Park, MD |
Area:
Astronomy and AstrophysicsGoogle:
"Rahul Shetty"Parents
Sign in to add mentor| Eve Charis Ostriker | grad student | 2007 | University of Maryland | |
| (Gas kinematics and dynamics: Spiral structure and cloud formation in disk galaxies.) | ||||
| Stuart N. Vogel | grad student | 2007 | University of Maryland (Physics Tree) | |
| Alyssa A. Goodman | post-doc | 2007-2010 | Harvard (Physics Tree) | |
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Publications
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| Peñaloza CH, Clark PC, Glover SCO, et al. (2017) Using CO line ratios to trace the physical properties of molecular clouds Monthly Notices of the Royal Astronomical Society. 465: 2277-2285 |
| Shetty R, Roman-Duval J, Hony S, et al. (2016) Simultaneously modelling far-infrared dust emission and its relation to CO emission in star-forming galaxies Monthly Notices of the Royal Astronomical Society. 460: 67-81 |
| Konstandin L, Schmidt W, Girichidis P, et al. (2016) Mach number study of supersonic turbulence: the properties of the density field Monthly Notices of the Royal Astronomical Society. 460: 4483-4491 |
| Stanchev O, Veltchev TV, Kauffmann J, et al. (2015) Tracing the general structure of Galactic molecular clouds using Planck data - I. The Perseus region as a test case Monthly Notices of the Royal Astronomical Society. 451: 1056-1069 |
| Bertram E, Konstandin L, Shetty R, et al. (2015) Centroid velocity statistics of molecular clouds Monthly Notices of the Royal Astronomical Society. 446: 3777-3787 |
| Konstandin L, Shetty R, Girichidis P, et al. (2015) Hierarchical Bayesian analysis of the velocity power spectrum in supersonic turbulence Monthly Notices of the Royal Astronomical Society. 446: 1775-1783 |
| Shetty R, Clark PC, Klessen RS. (2014) Interpreting the sub-linear Kennicutt-Schmidt relationship: The case for diffuse molecular gas Monthly Notices of the Royal Astronomical Society. 442: 2208-2215 |
| Bertram E, Shetty R, Glover SCO, et al. (2014) Principal component analysis of molecular clouds: Can CO reveal the dynamics? Monthly Notices of the Royal Astronomical Society. 440: 465-475 |
| Chira RA, Smith RJ, Klessen RS, et al. (2014) Line profiles of cores within clusters-III. What is the most reliable tracer of core collapse in dense clusters? Monthly Notices of the Royal Astronomical Society. 444: 874-886 |
| Lee MY, Stanimirović S, Wolfire MG, et al. (2014) The co-to-h2 conversion factor across the Perseus molecular cloud Astrophysical Journal. 784 |