M
Michael W. Werner
Researcher at California Institute of Technology
Publications - 394
Citations - 25116
Michael W. Werner is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Galaxy & Spitzer Space Telescope. The author has an hindex of 76, co-authored 392 publications receiving 23814 citations. Previous affiliations of Michael W. Werner include Ames Research Center & W.M. Keck Observatory.
Papers
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Journal ArticleDOI
Metallicity effects on dust properties in starbursting galaxies
Charles W. Engelbracht,George H. Rieke,Karl D. Gordon,J. D. T. Smith,Michael W. Werner,John Moustakas,Christopher N. A. Willmer,Leonardo Vanzi,Leonardo Vanzi +8 more
TL;DR: In this article, the authors present infrared observations of 66 starburst galaxies over the full range of oxygen abundances observed in local star-forming galaxies, from -->12 + log (O/H) = 7.1 to 8.9.
Journal ArticleDOI
Metallicity Effects on Mid-Infrared Colors and the 8 μm PAH Emission in Galaxies
Charles W. Engelbracht,Karl D. Gordon,George H. Rieke,Michael W. Werner,Daniel A. Dale,William B. Latter +5 more
TL;DR: In this article, the authors examined colors from 3.6 to 24 μm as a function of metallicity (O/H) for a sample of 34 galaxies and demonstrated that the shift is primarily due to a decrease in the 8 μm-to-24 μm color for metallicities between one-third and one-fifth of the solar value.
Journal ArticleDOI
C60 in reflection nebulae
Kris Sellgren,Michael W. Werner,James G. Ingalls,J. D. T. Smith,T. M. Carleton,Christine Joblin,Christine Joblin +6 more
TL;DR: In this article, the spectral properties of the fullerene C_(60) in the reflection nebula NGC 7023 were confirmed by detecting a third emission feature at 7.04 ± 0.05 μm.
Journal ArticleDOI
Molecular Hydrogen in H i Regions
Journal ArticleDOI
C$_{60}$ in Reflection Nebulae
Kris Sellgren,Michael W. Werner,James G. Ingalls,J. D. T. Smith,T. M. Carleton,Christine Joblin +5 more
TL;DR: In this article, the spectral properties of neutral C$60$ in the interstellar medium were confirmed by detecting a third emission feature at 7.04 $pm$ 0.05 $m in the reflection nebula NGC 7023.