Materials Map

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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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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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in Cooperation with on an Cooperation-Score of 37%

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Publications (1/1 displayed)

  • 2009The B0.5IVe CoRoT target HD 49330. I. Photometric analysis from CoRoT data101citations

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Emilio, M.
1 / 1 shared
Samadi, R.
1 / 1 shared
De Batz, B.
1 / 1 shared
Fabregat, J.
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Diago, P. D.
1 / 1 shared
Janot-Pacheco, E.
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Huat, A. -L.
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Hubert, A. -M.
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Baudin, F.
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Floquet, M.
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Michel, E.
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Frémat, Y.
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Gutiérrez-Soto, J.
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Neiner, Coralie
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Catala, C.
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Auvergne, M.
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Andrade, L.
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Leroy, B.
1 / 1 shared
Martayan, C.
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Semaan, T.
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Suso, J.
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2009

Co-Authors (by relevance)

  • Emilio, M.
  • Samadi, R.
  • De Batz, B.
  • Fabregat, J.
  • Diago, P. D.
  • Janot-Pacheco, E.
  • Huat, A. -L.
  • Hubert, A. -M.
  • Baudin, F.
  • Floquet, M.
  • Michel, E.
  • Frémat, Y.
  • Gutiérrez-Soto, J.
  • Neiner, Coralie
  • Catala, C.
  • Auvergne, M.
  • Andrade, L.
  • Leroy, B.
  • Martayan, C.
  • Semaan, T.
  • Suso, J.
OrganizationsLocationPeople

article

The B0.5IVe CoRoT target HD 49330. I. Photometric analysis from CoRoT data

  • Emilio, M.
  • Samadi, R.
  • Espinosa Lara, F.
  • De Batz, B.
  • Fabregat, J.
  • Diago, P. D.
  • Janot-Pacheco, E.
  • Huat, A. -L.
  • Hubert, A. -M.
  • Baudin, F.
  • Floquet, M.
  • Michel, E.
  • Frémat, Y.
  • Gutiérrez-Soto, J.
  • Neiner, Coralie
  • Catala, C.
  • Auvergne, M.
  • Andrade, L.
  • Leroy, B.
  • Martayan, C.
  • Semaan, T.
  • Suso, J.
Abstract

Context: Be stars undergo outbursts producing a circumstellar disk from the ejected material. The beating of non-radial pulsations has been put forward as a possible mechanism of ejection.<BR />Aims: We analyze the pulsational behavior of the early B0.5IVe star HD 49330 observed during the first CoRoT long run towards the Galactical anticenter (LRA1). This Be star is located close to the lower edge of the β Cephei instability strip in the HR diagram and showed a 0.03 mag outburst during the CoRoT observations. It is thus an ideal case for testing the aforementioned hypothesis.<BR />Methods: We analyze the CoRoT light curve of HD 49330 using Fourier methods and non-linear least square fitting. <BR />Results: In this star, we find pulsation modes typical of β Cep stars (p modes) and SPB stars (g modes) with amplitude variations along the run directly correlated with the outburst. These results provide new clues about the origin of the Be phenomenon as well as strong constraints on the seismic modelling of Be stars.Tables 3 to 7 are only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/506/95

Topics
  • impedance spectroscopy