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Spitzer observations of supernova remnants: II. Physical conditions and comparison with HH7 and HH54
molecular — ISM abundance — ISM clouds molecular processes shock waves
2010/11/9
We have studied the shock-excited molecular regions associated with four supernova remnants (SNRs) — IC443C, W28, W44 and 3C391 — and two Herbig-Haro objects,HH7 and HH54, using Spitzer ’s Infrared Sp...
A MODIFIED THEORETICAL Sigma-D RELATION FOR SUPERNOVA REMNANTS：I. THE CASE OF CONSTANT TEMPERATURE WITHIN THE SUPERNOVA REMNANT
ISM supernova remnants-radiation mechanisms thermal-radio continuum ISM
2009/3/13
We present a modification of the theoretical Σ − D relation for
supernova remnants (SNRs) in the adiabatic expansion phase. This modification
is based on the convolution of the relation first ...
RADIO-CONTINUUM STUDY OF THE SUPERNOVA REMNANTS IN THE LARGE MAGELLANIC CLOUD-AN SNR WITH A HIGHLY POLARISED BREAKOUT REGION-SNR J0455-6838
ISM supernova remnants-Magellanic Clouds-Radio Continuum ISM-Polarization-ISM individual objects-SNR J0455-6838
2009/1/19
We present the results of new moderate resolution ATCA obser-
vations of SNR J0455{6838. We found that this SNR exhibits a mostly typical
appearance with rather steep and curved ®={0.81§0.18 and...