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Mark G. Wolfire

Researcher at University of Maryland, College Park

Publications -  160
Citations -  19382

Mark G. Wolfire is an academic researcher from University of Maryland, College Park. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 57, co-authored 152 publications receiving 17615 citations. Previous affiliations of Mark G. Wolfire include Towson University & University of Chicago.

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The CO-to-H2 Conversion Factor

TL;DR: In this article, the authors review the theoretical underpinning, techniques, and results of efforts to estimate the CO-to-H2 conversion factor in different environments, and recommend a conversion factor XCO = 2×10 20 cm −2 (K km s −1 ) −1 with ±30% uncertainty.
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GLIMPSE. I. An SIRTF Legacy Project to Map the Inner Galaxy

TL;DR: The Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (GLIMPSE), a Space Infrared Telescope Facility (SIRTF) Legacy Science Program, will be a fully sampled, confusion-limited infrared survey of the inner Galactic disk with a pixel resolution of ∼1 as mentioned in this paper.
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GLIMPSE: I. A SIRTF Legacy Project to Map the Inner Galaxy

TL;DR: Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (GLIMPSE) as discussed by the authors is a collection of images collected by the SIRTF Legacy Science Program with a pixel resolution of 1.2" using the Infrared Array Camera (IRAC).
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Neutral Atomic Phases of the Interstellar Medium in the Galaxy

TL;DR: In this paper, the authors provided an analytic approximation for Pmin as a function of metallicity, far-ultraviolet radiation field, and the ionization rate of atomic hydrogen.