Stanley F. Dermott
Affiliations: | University of Florida, Gainesville, Gainesville, FL, United States |
Area:
Astronomy and AstrophysicsWebsite:
http://www.astro.ufl.edu/people/profiles/dermott.htmlGoogle:
"Stanley Dermott"Mean distance: 13552
Children
Sign in to add traineeRenu Malhotra | grad student | ||
Timothy Spahr | grad student | UF Gainesville | |
Elizabeth Katherine Holmes | grad student | 2002 | UF Gainesville (Astronomy Tree) |
Steven J. Novotny | grad student | 2003 | UF Gainesville |
Ashley J. Espy | grad student | 2009 | UF Gainesville |
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Publications
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Dermott SF, Christou AA, Li D, et al. (2018) The common origin of family and non-family asteroids Nature Astronomy. 2: 549-554 |
Kehoe AJE, Kehoe TJJ, Colwell JE, et al. (2015) SIGNATURES of RECENT ASTEROID DISRUPTIONS in the FORMATION and EVOLUTION of SOLAR SYSTEM DUST BANDS Astrophysical Journal. 811 |
Krüger H, Bindschadler D, Dermott SF, et al. (2010) Galileo dust data from the jovian system: 2000 to 2003 Planetary and Space Science. 58: 965-993 |
Krüger H, Dikarev V, Anweiler B, et al. (2010) Three years of Ulysses dust data: 2005 to 2007 Planetary and Space Science. 58: 951-964 |
Espy AJ, Dermott SF, Kehoe TJJ, et al. (2009) Evidence from IRAS for a very young, partially formed dust band Planetary and Space Science. 57: 235-242 |
Espy AJ, Dermott SF, Kehoe TJJ. (2008) Dynamical effects of mars on asteroidal dust particles Earth, Moon and Planets. 102: 199-203 |
Kehoe TJJ, Dermott SF, Mahoney-Hopping LM. (2007) The effect of inter-particle collisions on the dynamical evolution of asteroidal dust and the structure of the zodiacal cloud Esa - Workshop On Dust in Planetary Systems. 81-85 |
Krüger H, Altobelli N, Anweiler B, et al. (2006) Five years of Ulysses dust data: 2000-2004 Planetary and Space Science. 54: 932-956 |
Krüger H, Bindschadler D, Dermott SF, et al. (2006) Galileo dust data from the jovian system: 1997-1999 Planetary and Space Science. 54: 879-910 |
Telesco CM, Fisher RS, Wyatt MC, et al. (2005) Mid-infrared images of beta Pictoris and the possible role of planetesimal collisions in the central disk. Nature. 433: 133-6 |