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A Dirty WindowObserving in the Dark: The Dust-Gas Connection

A Dirty Window: Observing in the Dark: The Dust-Gas Connection [Along with the gas there is a ubiquitous solid component of the diffuse medium, loosely referred to as dust. Its presence was first inferred by distance dependent chromatic extinction (reddening) of starlight. But with satellite observations in the ultraviolet and far infrared, its thermal properties, spatial distribution, and physical makeup have been inferred. In this chapter we discuss the measurement of dust and its relation to the diffuse atomic and molecular gas.] http://www.deepdyve.com/assets/images/DeepDyve-Logo-lg.png

A Dirty WindowObserving in the Dark: The Dust-Gas Connection

Part of the Astrophysics and Space Science Library Book Series (volume 442)
Springer Journals — Apr 9, 2017

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Publisher
Springer Berlin Heidelberg
Copyright
© Springer-Verlag GmbH Germany 2017
ISBN
978-3-662-54348-1
Pages
155 –183
DOI
10.1007/978-3-662-54350-4_6
Publisher site
See Chapter on Publisher Site

Abstract

[Along with the gas there is a ubiquitous solid component of the diffuse medium, loosely referred to as dust. Its presence was first inferred by distance dependent chromatic extinction (reddening) of starlight. But with satellite observations in the ultraviolet and far infrared, its thermal properties, spatial distribution, and physical makeup have been inferred. In this chapter we discuss the measurement of dust and its relation to the diffuse atomic and molecular gas.]

Published: Apr 9, 2017

Keywords: Molecular Cloud; Column Density; Color Excess; Diffuse Medium; High Galactic Latitude

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