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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.

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Spitzer Observations of Bok Globule B335: Isolated Star Formation Efficiency and Cloud Structure

TL;DR: In this article, infrared and millimeter observations of Barnard 335, the prototypical isolated Bok globule with an embedded protostar, were used to measure the source luminosity accurately and constrain the density profile of the innermost globule material near the protostars using the observation of an 8.0 um shadow.
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Spatially Resolved Observations of the Galactic Center Source IRS 21

TL;DR: In this paper, diffraction-limited 2-25 μm images were obtained with the W. M. Keck 10 m telescopes that spatially resolved the cool source IRS 21, one of a small group of enigmatic objects in the central parsec of our Galaxy that have eluded classification.
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Do the Infrared Emission Features Need Ultraviolet Excitation

TL;DR: In this paper, the results of imaging spectroscopy of the reflection nebula vdB 133, obtained with the infrared camera and circular variable filter wheel on the Infrared Space Observatory, reveal the infrared emission features (IEFs), at 6.2, 7.7, 8.3, and 12.7 μm.
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Mid-infrared images of the debris disk around HD 141569

TL;DR: In this article, the authors used the Keck II telescope to image the debris disk around the A0 Ve/B95 Ve star HD 141569 (D = 99 pc), at λ = 125, 179, and 208 μm.