Analysis of the Hungaria asteroid population
暂无分享,去创建一个
Alan W. Harris | William F. Bottke | David Vokrouhlický | D. Vokrouhlický | W. Bottke | A. Harris | B. Warner | D. Nesvorný | David Nesvorný | Brian D. Warner
[1] Petr Pravec,et al. Binary asteroid population 1. Angular momentum content , 2007 .
[2] Andrew Scott Rivkin,et al. Yarkovsky footprints in the Eos family , 2006 .
[3] Alessandro Morbidelli,et al. Proper elements for highly inclined asteroidal orbits , 1994 .
[4] Robert Jedicke,et al. Linking the collisional history of the main asteroid belt to its dynamical excitation and depletion , 2005 .
[5] William F. Bottke,et al. THE YARKOVSKY AND YORP EFFECTS: Implications for Asteroid Dynamics , 2006 .
[7] K. Tsiganis,et al. Origin of the cataclysmic Late Heavy Bombardment period of the terrestrial planets , 2005, Nature.
[8] Andrea Milani,et al. Asteroid Proper Elements and the Dynamical Structure of the Asteroid Main Belt , 1994 .
[9] Alan W. Iarris. Tumbling Asteroids , 1997 .
[10] R. Gil-Hutton,et al. Collisional evolution of small body populations , 2002 .
[11] J. Henrard,et al. Secular resonances in the asteroid belt: Theoretical perturbation approach and the problem of their location , 1991 .
[12] Richard P. Binzel,et al. Phase II of the Small Main-Belt Asteroid Spectroscopic Survey: The Observations , 2002 .
[13] Petr Pravec,et al. The asteroid lightcurve database , 2009 .
[14] R. Gil-Hutton,et al. Polarimetric observations of Hungaria asteroids , 2007 .
[15] K. Tsiganis,et al. Origin of the orbital architecture of the giant planets of the Solar System , 2005, Nature.
[16] M. Nolan,et al. Velocity Distributions among Colliding Asteroids , 1994 .
[17] F. Marzari,et al. Computing the effects of YORP on the spin rate distribution of the NEO population , 2009 .
[18] D. Vokrouhlický,et al. The Effect of Yarkovsky Thermal Forces on the Dynamical Evolution of Asteroids and Meteoroids , 2002 .
[19] J. S. Dohnanyi. Collisional model of asteroids and their debris , 1969 .
[20] C. Chapman,et al. Families of minor planets , 1979 .
[21] Alessandro Morbidelli,et al. The Flora Family: A Case of the Dynamically Dispersed Collisional Swarm? , 2002 .
[22] Richard P. Binzel,et al. Phase II of the Small Main-Belt Asteroid Spectroscopic Survey: A Feature-Based Taxonomy , 2002 .
[23] P. Michel,et al. Rotational breakup as the origin of small binary asteroids , 2008, Nature.
[24] William F. Bottke,et al. An asteroid breakup 160 Myr ago as the probable source of the K/T impactor , 2007, Nature.
[25] The (not so) peculiar case of the Padua family , 2009 .
[26] The formation of asteroid satellites in cata-strophic impacts: results from numerical simulations , 2003 .
[27] Robert Jedicke,et al. The fossilized size distribution of the main asteroid belt , 2003 .
[28] Robert Jedicke,et al. Evidence for asteroid space weathering from the Sloan Digital Sky Survey , 2005 .
[29] Alain Doressoundiram,et al. Spectroscopic Properties of Asteroid Families , 2002 .
[30] Z. Ivezic,et al. Solar system objects observed in the Sloan Digital Sky Survey commissioning data , 2001 .
[31] D. J. Tholen,et al. Asteroid taxonomic classifications , 1989 .
[32] The Common Roots of Asteroids (6070) Rheinland and (54827) 2001 NQ8 , 2009 .
[33] J. Carvano,et al. Spectroscopic Survey of the Hungaria and Phocaea Dynamical Groups , 2001 .
[34] David Vokrouhlický,et al. PAIRS OF ASTEROIDS PROBABLY OF A COMMON ORIGIN , 2008 .
[35] V. Carruba,et al. A frequency approach to identifying asteroid families , 2007 .
[36] R. Gil-Hutton,et al. Surface composition of Hungaria asteroids from the analysis of the Sloan Digital Sky Survey colors , 2008 .
[37] Andrea Milani,et al. Asteroid proper elements and secular resonances , 1992 .
[38] Alessandro Morbidelli,et al. The peculiar case of the Agnia asteroid family , 2006 .
[39] Alessandro Morbidelli,et al. Iron meteorites as remnants of planetesimals formed in the terrestrial planet region , 2006, Nature.
[40] M. Ćuk,et al. Dynamical evolution of the Hungaria asteroids , 2009 .
[41] D. Vokrouhlický,et al. Spin rate distribution of small asteroids , 2008 .
[42] Yarkovsky Effect and the Dynamics of the Solar System , 2006 .
[43] Alberto Cellino,et al. Physical and Dynamical Properties of Asteroid Families , 2002 .
[44] D. Vokrouhlický,et al. The YORP effect with finite thermal conductivity , 2004 .
[45] Alessandro Morbidelli,et al. Yarkovsky/YORP chronology of asteroid families , 2006 .
[46] D. Vokrouhlický,et al. Express delivery of fossil meteorites from the inner asteroid belt to Sweden , 2007 .
[47] Stephan D. Price,et al. The Supplemental IRAS Minor Planet Survey , 2002 .
[48] Zeljko Ivezic,et al. The Size Distributions of Asteroid Families in the SDSS Moving Object Catalog 4 , 2008, 0807.3762.
[49] Anne Lemaitre,et al. Hungaria: A Potential New Family , 1994 .
[50] D. Vokrouhlický,et al. Dynamical Spreading of Asteroid Families by the Yarkovsky Effect , 2001, Science.