Jacob B. Simon, Ph.D.
Affiliations: | 2010 | University of Virginia, Charlottesville, VA |
Area:
Astronomy and AstrophysicsGoogle:
"Jacob Simon"Mean distance: 5668
Parents
Sign in to add mentor| John F. Hawley | grad student | 2010 | UVA | |
| (Local simulations of magnetized accretion disks.) | ||||
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Publications
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| Flaherty K, Hughes AM, Simon JB, et al. (2020) Measuring Turbulent Motion in Planet-forming Disks with ALMA: A Detection around DM Tau and Nondetections around MWC 480 and V4046 Sgr The Astrophysical Journal. 895: 109 |
| Fu RR, Kehayias P, Weiss BP, et al. (2020) Weak Magnetic Fields in the Outer Solar Nebula Recorded in CR Chondrites Journal of Geophysical Research. 125 |
| Li R, Youdin AN, Simon JB. (2019) Demographics of Planetesimals Formed by the Streaming Instability The Astrophysical Journal. 885: 69 |
| Abod CP, Simon JB, Li R, et al. (2019) The Mass and Size Distribution of Planetesimals Formed by the Streaming Instability. II. The Effect of the Radial Gas Pressure Gradient The Astrophysical Journal. 883: 192 |
| Mishra B, Begelman MC, Armitage PJ, et al. (2019) Strongly magnetized accretion discs: structure and accretion from global magnetohydrodynamic simulations Monthly Notices of the Royal Astronomical Society. 492: 1855-1868 |
| Nesvorný D, Li R, Youdin AN, et al. (2019) Trans-Neptunian binaries as evidence for planetesimal formation by the streaming instability Nature Astronomy. 3: 808-812 |
| Gole DA, Simon JB. (2018) The Nature of Turbulence in the Outer Regions of Protoplanetary Disks The Astrophysical Journal. 869: 84 |
| Simon JB, Bai X, Flaherty KM, et al. (2018) Origin of Weak Turbulence in the Outer Regions of Protoplanetary Disks The Astrophysical Journal. 865: 10 |
| Flaherty KM, Hughes AM, Teague R, et al. (2018) Turbulence in the TW Hya Disk The Astrophysical Journal. 856: 117 |
| Flaherty KM, Hughes AM, Rose SC, et al. (2017) A Three-dimensional View of Turbulence: Constraints on Turbulent Motions in the HD 163296 Protoplanetary Disk Using DCO+ The Astrophysical Journal. 843: 150 |