Materials Map

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

  • About
  • Privacy Policy
  • Legal Notice
  • Contact

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.

×

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.

To Graph

1.080 Topics available

To Map

977 Locations available

693.932 PEOPLE
693.932 People People

693.932 People

Show results for 693.932 people that are selected by your search filters.

←

Page 1 of 27758

→
←

Page 1 of 0

→
PeopleLocationsStatistics
Naji, M.
  • 2
  • 13
  • 3
  • 2025
Motta, Antonella
  • 8
  • 52
  • 159
  • 2025
Aletan, Dirar
  • 1
  • 1
  • 0
  • 2025
Mohamed, Tarek
  • 1
  • 7
  • 2
  • 2025
Ertürk, Emre
  • 2
  • 3
  • 0
  • 2025
Taccardi, Nicola
  • 9
  • 81
  • 75
  • 2025
Kononenko, Denys
  • 1
  • 8
  • 2
  • 2025
Petrov, R. H.Madrid
  • 46
  • 125
  • 1k
  • 2025
Alshaaer, MazenBrussels
  • 17
  • 31
  • 172
  • 2025
Bih, L.
  • 15
  • 44
  • 145
  • 2025
Casati, R.
  • 31
  • 86
  • 661
  • 2025
Muller, Hermance
  • 1
  • 11
  • 0
  • 2025
Kočí, JanPrague
  • 28
  • 34
  • 209
  • 2025
Šuljagić, Marija
  • 10
  • 33
  • 43
  • 2025
Kalteremidou, Kalliopi-ArtemiBrussels
  • 14
  • 22
  • 158
  • 2025
Azam, Siraj
  • 1
  • 3
  • 2
  • 2025
Ospanova, Alyiya
  • 1
  • 6
  • 0
  • 2025
Blanpain, Bart
  • 568
  • 653
  • 13k
  • 2025
Ali, M. A.
  • 7
  • 75
  • 187
  • 2025
Popa, V.
  • 5
  • 12
  • 45
  • 2025
Rančić, M.
  • 2
  • 13
  • 0
  • 2025
Ollier, Nadège
  • 28
  • 75
  • 239
  • 2025
Azevedo, Nuno Monteiro
  • 4
  • 8
  • 25
  • 2025
Landes, Michael
  • 1
  • 9
  • 2
  • 2025
Rignanese, Gian-Marco
  • 15
  • 98
  • 805
  • 2025

Fazio, G. G.

  • Google
  • 3
  • 47
  • 52

in Cooperation with on an Cooperation-Score of 37%

Topics

Publications (3/3 displayed)

  • 2015SOFIA/FORCAST Observations of Warm Dust in S106: A Fragmented Environment5citations
  • 2014PdBI Cold Dust Imaging of Two Extremely Red H - [4.5] 〉 4 Galaxies Discovered with SEDS and CANDELS12citations
  • 2010Anomalous Silicate Dust Emission in the Type 1 Liner Nucleus of M8135citations

Places of action

Chart of shared publication
Dunlop, J. S.
1 / 1 shared
Santini, P.
1 / 3 shared
Fontana, A.
1 / 4 shared
Ashby, M. L. N.
2 / 3 shared
Caputi, K. I.
1 / 3 shared
Michałowski, M. J.
1 / 1 shared
Huang, J. -S.
2 / 2 shared
Krips, M.
1 / 1 shared
Geach, J. E.
1 / 1 shared
Koekemoer, A. M.
1 / 1 shared
Popping, G.
1 / 1 shared
Castellano, Marco
1 / 1 shared
Spaans, M.
1 / 1 shared
Marengo, M.
1 / 6 shared
Zezas, A.
1 / 1 shared
Wu, Y. L.
1 / 1 shared
Willner, S.
1 / 1 shared
Smith, Howard A.
1 / 2 shared
Köhler, M.
1 / 10 shared
Li, Aigen
1 / 1 shared
Li, M. P.
1 / 1 shared
Spinoglio, Luigi
1 / 4 shared
Wang, Z.
1 / 99 shared
Chart of publication period
2015
2014
2010

Co-Authors (by relevance)

  • Dunlop, J. S.
  • Santini, P.
  • Fontana, A.
  • Ashby, M. L. N.
  • Caputi, K. I.
  • Michałowski, M. J.
  • Huang, J. -S.
  • Krips, M.
  • Geach, J. E.
  • Koekemoer, A. M.
  • Popping, G.
  • Castellano, Marco
  • Spaans, M.
  • Marengo, M.
  • Zezas, A.
  • Wu, Y. L.
  • Willner, S.
  • Smith, Howard A.
  • Köhler, M.
  • Li, Aigen
  • Li, M. P.
  • Spinoglio, Luigi
  • Wang, Z.
OrganizationsLocationPeople

article

SOFIA/FORCAST Observations of Warm Dust in S106: A Fragmented Environment

  • Koenig, X. P.
  • Hankins, M.
  • Kraemer, K. E.
  • Allen, L. E.
  • Keto, E.
  • Mizuno, D. R.
  • Myers, P. C.
  • Gutermuth, R. A.
  • Staguhn, J. G.
  • Herter, T. L.
  • Hill, T.
  • Smith, N.
  • Gehrz, R. D.
  • Hora, J. L.
  • Carey, Sean
  • Guzman Fernandez, A.
  • Fazio, G. G.
  • Bontemps, S.
  • Lau, R. M.
  • Simon, R.
  • Motte, F.
  • Smith, H. A.
  • Adams, J. D.
  • Schneider, N.
  • Megeath, S. T.
Abstract

We present mid-IR (19-37 μm) imaging observations of S106 from SOFIA/FORCAST, complemented with IR observations from Spitzer/IRAC (3.6-8.0 μm), IRTF/MIRLIN (11.3 and 12.5 μm), and Herschel/PACS (70 and 160 μm). We use these observations, observations in the literature, and radiation transfer modeling to study the heating and composition of the warm (̃100 K) dust in the region. The dust is heated radiatively by the source S106 IR, with little contributions from grain-electron collisions and Lyα radiation. The dust luminosity is ≳(9.02 ± 1.01) × 10<SUP>4</SUP> L<SUB>☉</SUB>, consistent with heating by a mid- to late-type O star. We find a temperature gradient (̃75-107 K) in the lobes, which is consistent with a dusty equatorial geometry around S106 IR. Furthermore, the SOFIA observations resolve several cool (̃65-70 K) lanes and pockets of warmer (̃75-90 K) dust in the ionization shadow, indicating that the environment is fragmented. We model the dust mass as a composition of amorphous silicates, amorphous carbon, big grains, very small grains, and polycyclic aromatic hydrocarbons. We present the relative abundances of each grain component for several locations in S106....

Topics
  • impedance spectroscopy
  • amorphous
  • Carbon
  • grain