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

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

Topics

Publications (6/6 displayed)

  • 2021JWST Survey of the Prototypical Core-collapse Supernova Remnant Cassiopeia Acitations
  • 2012A Detailed Chandra Study of the Interstellar Medium Metallicity in the Large Magellanic Cloudcitations
  • 2012Properties and Spatial Distribution of Dust Emission in the Crab Nebula46citations
  • 2008Discovery of Fast-Moving X-Ray-Emitting Ejecta Knots in the Oxygen-Rich Supernova Remnant Puppis A36citations
  • 2001Two New Ejecta-dominated Galactic Supernova Remnants: G337.2-0.7 and G309.2-0.625citations
  • 2001A New ASCA and ROSAT Study of the Supernova Remnant G272.2-3.227citations

Places of action

Chart of shared publication
Arendt, Richard G.
2 / 6 shared
Temim, Tea
2 / 3 shared
Mori, K.
2 / 6 shared
Boone, C.
1 / 1 shared
Schenck, Andrew
1 / 1 shared
Park, S.
2 / 18 shared
Lee, J.
1 / 41 shared
Lord, R.
1 / 1 shared
Burrows, D.
1 / 3 shared
Post, S.
1 / 1 shared
Hughes, John P.
2 / 5 shared
Dwek, Eli
1 / 10 shared
Roellig, Thomas L.
1 / 2 shared
Gehrz, Robert D.
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Sonneborn, George
1 / 3 shared
Katsuda, S.
1 / 2 shared
Tsunemi, H.
1 / 1 shared
Hwang, U.
1 / 1 shared
Burrows, D. N.
1 / 1 shared
Hughes, J. P.
2 / 2 shared
Rakowski, Cara E.
1 / 1 shared
Smith, R. K.
1 / 1 shared
Harrus, Ilana M.
1 / 1 shared
Chart of publication period
2021
2012
2008
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Co-Authors (by relevance)

  • Arendt, Richard G.
  • Temim, Tea
  • Mori, K.
  • Boone, C.
  • Schenck, Andrew
  • Park, S.
  • Lee, J.
  • Lord, R.
  • Burrows, D.
  • Post, S.
  • Hughes, John P.
  • Dwek, Eli
  • Roellig, Thomas L.
  • Gehrz, Robert D.
  • Sonneborn, George
  • Katsuda, S.
  • Tsunemi, H.
  • Hwang, U.
  • Burrows, D. N.
  • Hughes, J. P.
  • Rakowski, Cara E.
  • Smith, R. K.
  • Harrus, Ilana M.
OrganizationsLocationPeople

document

A Detailed Chandra Study of the Interstellar Medium Metallicity in the Large Magellanic Cloud

  • Mori, K.
  • Boone, C.
  • Schenck, Andrew
  • Park, S.
  • Lee, J.
  • Lord, R.
  • Burrows, D.
  • Slane, Patrick
  • Post, S.
  • Hughes, John P.
Abstract

Measurements of interstellar composition are essential for understanding galactic evolution and the star-formation history of the Milky Way and other nearby galaxies. The Large Magellanic Cloud (LMC) is an excellent candidate for the study of the Interstellar Medium (ISM) thanks to its proximity and low foreground absorption. X-ray spectroscopy of supernova remnants (SNRs) is independent of and complementary to the traditional optical spectroscopy of stars and HII regions for measuring metal abundances of gas-phase ISM. The LMC abundances currently available in the literature are based on data more than a decade-old. In particular, X-ray measurements were derived from a small number of SNRs observed by low resolution ( 3') ASCA detectors which were not able to avoid contamination from embedded metal-rich ejecta and/or pulsar wind nebulae. With high-resolution (0.5") Chandra data we can clearly isolate the swept-up ISM shells from central metal-rich ejecta and/or pulsar wind nebulae to estimate the 'true' metal abundances of the LMC ISM. Now, several dozens of LMC SNRs have been observed by Chandra, providing a large sample and diversity needed for accurate measurements of ISM abundances across the entire galaxy. We present our initial results on the O, Ne, Mg, Si, and Fe abundances of 17 LMC SNRs. We found our values to be typically lower than previously measured....

Topics
  • impedance spectroscopy
  • phase
  • X-ray spectroscopy