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AKARI NIR spectroscopy of interstellar ices
2015
Proceedings of the International Astronomical Union
The Infrared Camera (IRC) onboard AKARI has a near-infrared (2--5μm) spectroscopic capability with high sensitivity that allows us to study the major ice components in various objects. In particular, H2O and CO2 ice absorption features have been detected towards nearby galaxies, including several young stellar objects (YSOs) in the Large Magellanic Cloud (LMC), as well as a number of HII region-PDR complexes for the first time by IRC spectroscopy. While observations in the LMC show a high ratio
doi:10.1017/s1743921316003161
fatcat:czkxuvqrdvevnpxo5kyfxdnqca