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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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%

Topics

Publications (1/1 displayed)

  • 2006Spitzer MIPS Infrared Imaging of M31: Further Evidence for a Spiral-Ring Composite Structure166citations

Places of action

Chart of shared publication
Young, E. T.
1 / 1 shared
Engelbracht, C. W.
1 / 3 shared
Gibson, B. K.
1 / 1 shared
Rieke, G. H.
1 / 4 shared
Barmby, P.
1 / 1 shared
Misselt, K. A.
1 / 5 shared
Marleau, F. R.
1 / 1 shared
Hinz, J.
1 / 3 shared
Bailin, J.
1 / 1 shared
Krause, O.
1 / 2 shared
Latter, W. B.
1 / 2 shared
Hines, D. C.
1 / 1 shared
Werner, M. W.
1 / 2 shared
Gordon, Karl
1 / 8 shared
Ashby, M. L. N.
1 / 3 shared
Thilker, D. A.
1 / 1 shared
Noriega-Crespo, A.
1 / 1 shared
Stolovy, S.
1 / 1 shared
Chart of publication period
2006

Co-Authors (by relevance)

  • Young, E. T.
  • Engelbracht, C. W.
  • Gibson, B. K.
  • Rieke, G. H.
  • Barmby, P.
  • Misselt, K. A.
  • Marleau, F. R.
  • Hinz, J.
  • Bailin, J.
  • Krause, O.
  • Latter, W. B.
  • Hines, D. C.
  • Werner, M. W.
  • Gordon, Karl
  • Ashby, M. L. N.
  • Thilker, D. A.
  • Noriega-Crespo, A.
  • Stolovy, S.
OrganizationsLocationPeople

article

Spitzer MIPS Infrared Imaging of M31: Further Evidence for a Spiral-Ring Composite Structure

  • Young, E. T.
  • Engelbracht, C. W.
  • Gibson, B. K.
  • Rieke, G. H.
  • Barmby, P.
  • Misselt, K. A.
  • Levine, D. A.
  • Marleau, F. R.
  • Hinz, J.
  • Bailin, J.
  • Krause, O.
  • Latter, W. B.
  • Hines, D. C.
  • Werner, M. W.
  • Gordon, Karl
  • Ashby, M. L. N.
  • Thilker, D. A.
  • Noriega-Crespo, A.
  • Stolovy, S.
Abstract

New images of M31 at 24, 70, and 160 μm taken with the Multiband Imaging Photometer for Spitzer (MIPS) reveal the morphology of the dust in this galaxy. This morphology is well represented by a composite of two logarithmic spiral arms and a circular ring (radius ~10 kpc) of star formation offset from the nucleus. The two spiral arms appear to start at the ends of a bar in the nuclear region and extend beyond the star-forming ring. As has been found in previous work, the spiral arms are not continuous, but composed of spiral segments. The star-forming ring is very circular except for a region near M32 where it splits. The lack of well-defined spiral arms and the prominence of the nearly circular ring suggest that M31 has been distorted by interactions with its satellite galaxies. Using new dynamical simulations of M31 interacting with M32 and NGC 205, we find that, qualitatively, such interactions can produce an offset, split ring like that seen in the MIPS images.

Topics
  • impedance spectroscopy
  • morphology
  • simulation
  • composite
  • forming