Physical characterization of the near-Earth object population

S. Ieva; E. Dotto; E. Mazzotta Epifani; D. Perna; E. Perozzi; M. Micheli

doi:10.1140/epjp/i2017-11622-6

Journal Articles The European Physical Journal Plus Year : 2017

Physical characterization of the near-Earth object population

(1) , (1) , (1) , (2, 3) , ,

1
2
3

S. Ieva

Function : Author

INAF - Osservatorio Astronomico di Roma

E. Dotto

Function : Author

INAF - Osservatorio Astronomico di Roma

E. Mazzotta Epifani

Function : Author

INAF - Osservatorio Astronomico di Roma

D. Perna

Function : Author
PersonId : 762869
ORCID : 0000-0002-4545-3850
IdRef : 147151708

Università degli Studi di Roma Tor Vergata [Roma, Italia] = University of Rome Tor Vergata [Rome, Italy] = Université de Rome Tor Vergata [Rome, Italie]

Laboratoire d'études spatiales et d'instrumentation en astrophysique

E. Perozzi

Function : Author

M. Micheli

Function : Author

Domains

Physics [physics] Astrophysics [astro-ph]

la. bibliotheque : Connect in order to contact the contributor

https://hal-obspm.ccsd.cnrs.fr/obspm-02194448

Submitted on : Thursday, July 25, 2019-3:08:35 PM

Last modification on : Monday, May 13, 2024-10:56:02 AM

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obspm-02194448 , version 1 (25-07-2019)

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HAL Id : obspm-02194448 , version 1
DOI : 10.1140/epjp/i2017-11622-6

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S. Ieva, E. Dotto, E. Mazzotta Epifani, D. Perna, E. Perozzi, et al.. Physical characterization of the near-Earth object population. The European Physical Journal Plus, 2017, 132 (8), ⟨10.1140/epjp/i2017-11622-6⟩. ⟨obspm-02194448⟩

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Physical characterization of the near-Earth object population

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