Mid-IR spectroscopy of low metallicity galaxies with Spitzer/IRS

Details Mid-IR spectroscopy of low metallicity galaxies with Spitzer/IRS Mid-IR spectroscopy of low metallicity galaxies with Spitzer/IRS

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..357..208h&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 infrared spectrograph, IRS, on the Spitzer Space Telescope has greatly improved the sensitivity in the thermal infrared and opened many new avenues in infrared astronomy over the range of 5.5 to 38 microns. With the IRS an object with midinfrared flux of ˜1 mJy can produce a usable low resolution spectrum in an hour of telescope time. The mid infrared study of star formation at low metallicity has been enabled by this new sensitivity.

Affiliated with

Also associated with

No associations

Rating

Mid-IR spectroscopy of low metallicity galaxies with Spitzer/IRS does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Mid-IR spectroscopy of low metallicity galaxies with Spitzer/IRS, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mid-IR spectroscopy of low metallicity galaxies with Spitzer/IRS will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1240842