Are the E-type asteroids (2867) Steins, a target of the Rosetta mission, and NEA (3103) Eger remnants of an old asteroid family?

Astronomy and Astrophysics

Volumn 474, Issue 2, 2007, Pages

  Fornasier, S ^a,b   Marzari, F ^c   Dotto, E ^d   Barucci, M A ^a   Migliorini, A ^e  

^a OBSERVATOIRE DE PARIS   (France)

^b UNIVERSITÉ PARIS DESCARTES   (France)

^c UNIVERSITY OF PADOVA   (Italy)

^d INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

^e INAF IASF ROMA   (Italy)

Author keywords

Methods: numerical; Methods: observational; Minor planets, asteroids; Techniques: spectroscopic

Indexed keywords

NUMERICAL METHODS; ORBITS; PLANETS; SPACE RESEARCH; SPECTROSCOPIC ANALYSIS;

EARTH-CROSSING ORBITS; MINOR PLANETS; NUMERICAL ORBITAL INTEGRATIONS;

ASTEROIDS;

EID: 35548935206     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078411     Document Type: Article

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