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  The 2.5-5.1 μm reflectance spectra of HED meteorites and their constituent minerals: Implications for Dawn

Cloutis, E. A., Mann, P., Izawa, M. R. M., Nathues, A., Reddy, V., Hiesinger, H., et al. (2013). The 2.5-5.1 μm reflectance spectra of HED meteorites and their constituent minerals: Implications for Dawn. Icarus, 225(1), 581-601. doi:10.1016/j.icarus.2013.04.022.

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 Creators:
Cloutis, E. A., Author
Mann, P., Author
Izawa, M. R. M., Author
Nathues, A.1, 2, Author              
Reddy, V.2, Author              
Hiesinger, H., Author
Le Corre, L.2, Author              
Palomba, E., Author
Affiliations:
1MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291              
2Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832288              

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 MPIS_PROJECTS: DAWN
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 Dates: 2013
 Publication Status: Published in print
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 Rev. Type: Peer
 Identifiers: DOI: 10.1016/j.icarus.2013.04.022
BibTex Citekey: Cloutis:2013-160
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Title: Icarus
Source Genre: Journal
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Pages: - Volume / Issue: 225 (1) Sequence Number: - Start / End Page: 581 - 601 Identifier: -