Infrared Observations of Shock-Cloud Interactions around Supernova Remnants

Details Infrared Observations of Shock-Cloud Interactions around Supernova Remnants Infrared Observations of Shock-Cloud Interactions around Supernova Remnants

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..418..471s&link_type=abstract

AKARI, a Light to Illuminate the Misty Universe ASP Conference Series, Vol. 418, proceedings of a conference held 16-19 February

Astronomy and Astrophysics

Astronomy

Scientific paper

The infrared wavelength region provides a useful window within which to study shock-cloud interactions, since it includes numerous diagnostic ionic and molecular lines. Many of these radiative signatures occur at mid-infrared wavelengths, where ground observations are impossible because of intense atmospheric absorption. Hence, space observatories, e.g., AKARI, are crucial in studying shock-cloud interactions. We present observations of interaction regions around two supernova remnants - HB21 and G272.2-3.2 - observed with AKARI, which we interpret as being due to shocked H2 and ionic emissions.

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