Materials Map

Discover the materials research landscape. Find experts, partners, networks.

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The Materials Map is an open tool for improving networking and interdisciplinary exchange within materials research. It enables cross-database search for cooperation and network partners and discovering of the research landscape.

The dashboard provides detailed information about the selected scientist, e.g. publications. The dashboard can be filtered and shows the relationship to co-authors in different diagrams. In addition, a link is provided to find contact information.

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Materials Map under construction

The Materials Map is still under development. In its current state, it is only based on one single data source and, thus, incomplete and contains duplicates. We are working on incorporating new open data sources like ORCID to improve the quality and the timeliness of our data. We will update Materials Map as soon as possible and kindly ask for your patience.

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1.080 Topics available

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977 Locations available

693.932 PEOPLE
693.932 People People

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Naji, M.
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in Cooperation with on an Cooperation-Score of 37%

Topics

Publications (4/4 displayed)

  • 2019The Thermal, Mechanical, Structural, and Dielectric Properties of Cometary Nuclei After Rosetta91citations
  • 2017Cometary coma dust size distribution from in situ IR spectra17citations
  • 2003Unveiling the nature of 10199 Chariklo: near-infrared observations and modeling35citations
  • 2002A portrait of the Centaur 10199 Chariklocitations

Places of action

Chart of shared publication
Tosi, F.
1 / 5 shared
Ciarletti, V.
1 / 5 shared
Skorov, Y.
1 / 1 shared
Filacchione, G.
2 / 3 shared
Pelivan, I.
1 / 1 shared
Marshall, D.
1 / 1 shared
Knollenberg, J.
1 / 1 shared
Knapmeyer, M.
1 / 1 shared
Gundlach, B.
1 / 1 shared
Fischer, H.-H.
1 / 1 shared
Davidsson, B.
1 / 1 shared
Brouet, Y.
1 / 5 shared
Attree, N.
1 / 1 shared
Groussin, O.
1 / 2 shared
Snodgrass, Colin
1 / 1 shared
Kokotanekova, Rosita
1 / 1 shared
Kührt, E.
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Spohn, T.
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Capaccioni, F.
1 / 3 shared
Rinaldi, G.
1 / 1 shared
Della Corte, V.
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Ivanovski, S. L.
1 / 1 shared
Ciarniello, M.
1 / 5 shared
Palomba, E.
1 / 8 shared
Daversa, E.
1 / 2 shared
Tozzi, G. P.
1 / 1 shared
Rotundi, A.
1 / 3 shared
Erard, S.
1 / 1 shared
Taylor, F.
1 / 1 shared
Capria, M. T.
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Mottola, S.
1 / 2 shared
Salatti, M.
1 / 1 shared
Fulle, M.
1 / 2 shared
Bockelée-Morvan, D.
1 / 3 shared
Longobardo, Andrea
1 / 3 shared
Licandro, J.
2 / 2 shared
Dotto, Elisabetta
2 / 6 shared
Romon, J.
2 / 2 shared
Barucci, M. A.
2 / 8 shared
De Bergh, C.
2 / 5 shared
Chart of publication period
2019
2017
2003
2002

Co-Authors (by relevance)

  • Tosi, F.
  • Ciarletti, V.
  • Skorov, Y.
  • Filacchione, G.
  • Pelivan, I.
  • Marshall, D.
  • Knollenberg, J.
  • Knapmeyer, M.
  • Gundlach, B.
  • Fischer, H.-H.
  • Davidsson, B.
  • Brouet, Y.
  • Attree, N.
  • Groussin, O.
  • Snodgrass, Colin
  • Kokotanekova, Rosita
  • Kührt, E.
  • Spohn, T.
  • Capaccioni, F.
  • Rinaldi, G.
  • Della Corte, V.
  • Ivanovski, S. L.
  • Ciarniello, M.
  • Palomba, E.
  • Daversa, E.
  • Tozzi, G. P.
  • Rotundi, A.
  • Erard, S.
  • Taylor, F.
  • Capria, M. T.
  • Mottola, S.
  • Salatti, M.
  • Fulle, M.
  • Bockelée-Morvan, D.
  • Longobardo, Andrea
  • Licandro, J.
  • Dotto, Elisabetta
  • Romon, J.
  • Barucci, M. A.
  • De Bergh, C.
OrganizationsLocationPeople

article

Unveiling the nature of 10199 Chariklo: near-infrared observations and modeling

  • Licandro, J.
  • Dotto, Elisabetta
  • Romon, J.
  • Barucci, M. A.
  • De Bergh, C.
  • Leyrat, C.
Abstract

10199 Chariklo (1997 CU26) is the largest Centaur so far known. We carried out near-infrared observations of this object during two different runs separated by a year. Although no evidence for spectral variations has been found over short time scales, slight differences have been detected between the two observational runs. We interpret these findings as likely due to a heterogeneous composition of the surface of Chariklo. We suggest two different models comprising geographical mixtures of tholins, amorphous carbon, and water ice in slightly different percentages. Our observations confirm the presence of water ice on the surface of this Centaur, as already detected by Brown et al. (1998, Science 280, 1430-1432) and Brown and Koresko (1998, Astrophys. J. 505, L65-67)....

Topics
  • impedance spectroscopy
  • surface
  • amorphous
  • Carbon