TheSpitzer/GLIMPSE Surveys: A New View of the Milky Way

A brief description is given of the GLIMPSE surveys, including the areas surveyed, sensitivity limits, and products. The primary motivations for this review are to describe some of the main scientific results enabled by the GLIMPSE surveys and to note potential future applications of the GLIMPSE cat...

Full description

Saved in:
Bibliographic Details
Published inPublications of the Astronomical Society of the Pacific Vol. 121; no. 877; pp. 213 - 230
Main Authors Churchwell, Ed, Babler, Brian L., Meade, Marilyn R., Whitney, Barbara A., Benjamin, Robert, Indebetouw, Remy, Cyganowski, Claudia, Robitaille, Thomas P., Povich, Matthew, Watson, Christer, Bracker, Steve
Format Journal Article
LanguageEnglish
Japanese
Published University of Chicago Press 01.03.2009
Subjects
Online AccessGet full text

Cover

Loading…
More Information
Summary:A brief description is given of the GLIMPSE surveys, including the areas surveyed, sensitivity limits, and products. The primary motivations for this review are to describe some of the main scientific results enabled by the GLIMPSE surveys and to note potential future applications of the GLIMPSE catalogs and images. In particular, we discuss contributions to our understanding of star formation and early evolution, the interstellar medium, galactic structure, and evolved stars. Infrared dark clouds (IRDCs), young stellar objects (YSOs), and infrared bubbles/H IIregions are discussed in some detail. A probable triggered star formation associated with expanding infrared bubbles is briefly mentioned. The distribution and morphologies of dust and polycyclic aromatic hydrocarbons (PAHs) in the interstellar medium are discussed. Examples are shown from GLIMPSE images of bow shocks, pillars (elephant trunks), and instabilities in massive star-formation regions. The infrared extinction law of diffuse interstellar dust is discussed. The large-scale structure of the Galaxy has been traced by red-clump giants using the GLIMPSE point-source catalog to reveal the radius and orientation of the central bar, the stellar radial scale length, an obvious increase in star counts toward the tangency to the Scutum-Centaurus spiral arm, the lack of an obvious tangency from star counts toward the Sagittarius spiral arm, and a sharp increase in star counts toward the nuclear bulge. Recent results on evolved stars and some serendipitous discoveries are mentioned. More than 70 refereed papers have been published based on GLIMPSE data as of 2008 November.
ISSN:0004-6280
1538-3873
DOI:10.1086/597811