The statistical asteroid model. I. The main-belt population for diameters greater than 1 kilometer

Astronomical Journal

Volumn 129, Issue 6, 2005, Pages 2869-2886

  Tedesco, Edward F ^a   Cellino, Alberto ^b   Zapralá, Vincenzo ^b  

^a UNIVERSITY OF NEW HAMPSHIRE   (United States)

^b OSSERVATORIO ASTRONOMICO DI TORINO   (Italy)

Author keywords

Infrared: solar system; Minor planets, asteroids; Solar system: general

Indexed keywords

EID: 22544446749     PISSN: 00046256     EISSN: None     Source Type: Journal    
DOI: 10.1086/429734     Document Type: Article

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