Spitzer's Observations of the Small Magellanic Cloud: Probing the PAH Distribution

Details Spitzer's Observations of the Small Magellanic Cloud: Probing the PAH Distribution Spitzer's Observations of the Small Magellanic Cloud: Probing the PAH Distribution

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..357..162s&link_type=abstract

The Spitzer Space Telescope: New Views of the Cosmos ASP Conference Series, Volume 357, proceedings of the conference held 9-12

Astronomy and Astrophysics

Astronomy

Scientific paper

The Spitzer program to image the Small Magellanic Cloud (SMC) with all IRAC and MIPS bands is well underway. IRAC observations in particularly will allow, for the first time, to quantify the distribution and properties of very small dust grains and PAHs across the entire SMC, as well as to study their environmental dependence and preferences. In this paper we describe project goals and give a flavor of the 24μm observations by examining briefly the structure in one of the most oxygen-rich supernova remnants, E0102-7219.

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