Young SNRs: IR observations

Details Young SNRs: IR observations Young SNRs: IR observations

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..565..163a&link_type=abstract

YOUNG SUPERNOVA REMNANTS: Eleventh Astrophysics Conference. AIP Conference Proceedings, Volume 565, pp. 163-172 (2001).

Astronomy and Astrophysics

Astrophysics

Infrared, Pre-Main Sequence Objects, Young Stellar Objects And Protostars, Supernovae

Scientific paper

Infrared observations of SNRs began with the IRAS mission in 1983. Now as more detailed ISO and 2MASS observations of SNRs are being analyzed, we are beginning to see more clearly what the IR has to reveal. For young SNRs this has most notably meant a detailed look at SN ejecta before it is mixed into the ISM. The IR can reveal the presence of elements and gas phases that are undetectable at other wavelengths. The IR emission is also essential for identifying the particular composition and mineral structure of dust grains that form in the SN ejecta. .

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