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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693.932 PEOPLE
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in Cooperation with on an Cooperation-Score of 37%

Topics

Publications (4/4 displayed)

  • 2011The identification of probable SiS emission at 13-14 μm in spectra of galactic S stars9citations
  • 2007Luminosities and mass-loss rates of carbon stars in the Magellanic Clouds101citations
  • 2007Molecules and dust grains in AGB stars in nearby galaxies - The influence of metallicitiescitations
  • 2005An empirical formula for the mass-loss rates of dust-enshrouded red supergiants and oxygen-rich Asymptotic Giant Branch stars376citations

Places of action

Chart of shared publication
Zijlstra, Albert
4 / 15 shared
Feast, M. W.
3 / 7 shared
Groenewegen, M. A. T.
3 / 13 shared
Sahai, R.
1 / 5 shared
Sloan, G. C.
3 / 17 shared
Decin, L.
1 / 2 shared
Wyk, F. Van
1 / 1 shared
Smolders, K.
1 / 3 shared
Hony, S.
2 / 7 shared
Matsuura, M.
2 / 12 shared
Olivier, E. A.
1 / 2 shared
Cioni, M. R. L.
3 / 7 shared
Blommaert, J. A. D. L.
1 / 4 shared
Wood, P. R.
2 / 9 shared
Vanhollebeke, E.
1 / 2 shared
Lagadec, E.
2 / 7 shared
Menzies, J. W.
2 / 6 shared
Habing, H. J.
1 / 4 shared
Whitelock, P. A.
2 / 6 shared
Bernard-Salas, J.
1 / 8 shared
Harris, G. J.
1 / 2 shared
Loup, C.
1 / 3 shared
Chart of publication period
2011
2007
2005

Co-Authors (by relevance)

  • Zijlstra, Albert
  • Feast, M. W.
  • Groenewegen, M. A. T.
  • Sahai, R.
  • Sloan, G. C.
  • Decin, L.
  • Wyk, F. Van
  • Smolders, K.
  • Hony, S.
  • Matsuura, M.
  • Olivier, E. A.
  • Cioni, M. R. L.
  • Blommaert, J. A. D. L.
  • Wood, P. R.
  • Vanhollebeke, E.
  • Lagadec, E.
  • Menzies, J. W.
  • Habing, H. J.
  • Whitelock, P. A.
  • Bernard-Salas, J.
  • Harris, G. J.
  • Loup, C.
OrganizationsLocationPeople

article

The identification of probable SiS emission at 13-14 μm in spectra of galactic S stars

  • Zijlstra, Albert
  • Loon, J. Th Van
  • Feast, M. W.
  • Groenewegen, M. A. T.
  • Sahai, R.
  • Sloan, G. C.
  • Decin, L.
  • Wyk, F. Van
  • Smolders, K.
  • Hony, S.
Abstract

A sample of 90 Galactic S stars observed by the Spitzer Space Telescope includes two sources with unusual low-contrast spectral structure between 7 and 14 μm. The most likely estimate of the spectral continuum leads to the identification of molecular emission features from SiS at 7 and 13-14 μm. The spectra also show what is best described as featureless excess emission, most likely from iron dust but possibly from amorphous carbon, as well as an emission feature from amorphous alumina dust peaking at 11-12 μm. The spectra show long-wavelength excesses from cool dust grains in an extended envelope and additional emission features of unknown origin. © 2011. The American Astronomical Society. All rights reserved.

Topics
  • impedance spectroscopy
  • amorphous
  • Carbon
  • grain
  • iron