Dust Destruction in the Cygnus Loop Supernova Remnant
2013 ◽
Vol 9
(S296)
◽
pp. 160-164
◽
Keyword(s):
AbstractThe Cygnus Loop supernova remnant serves as an excellent laboratory for the study of radiative and non-radiative shocks with speeds in the 150–450 km s−1 range. We present results on shock-excited emission and dust destruction based on Spitzer Space Telescope observations of two well-studied regions in the remnant, (i) a non-radiative shock filament along the NE limb, and (ii) the XA region, characterized by emission from bright radiative shocks.
2010 ◽
Vol 712
(2)
◽
pp. 1092-1099
◽
2016 ◽
Vol 826
(2)
◽
pp. 150
◽
2007 ◽
Vol 59
(sp1)
◽
pp. S163-S170
◽
Keyword(s):