Nature of a Maser-Emitting and EGRET Source SNR: SNR-Molecular Cloud Interaction

Details Nature of a Maser-Emitting and EGRET Source SNR: SNR-Molecular Cloud Interaction Nature of a Maser-Emitting and EGRET Source SNR: SNR-Molecular Cloud Interaction

Sep 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005cxo..prop.1973n&link_type=abstract

Chandra Proposal ID #07500782

Computer Science

Chandra Proposal Id #07500782

Scientific paper

The interaction between supernova remnants (SNRs) and molecular clouds causes immediate heating and changes the chemical composition of the surrounding gas, emitting thermal and non-thermal X-rays, OH maser lines, and gamma-rays. However, what causes the partial overlap among maser-emitting SNRs, EGRET source SNRs, SNRs with particular X-ray properties such as mixed-morphology SNRs is still unclear. CTB 37A is a radio-bright Galactic SNR, and is accompanied by OH masers and EGRET source. As the best target for the study of the SNRs in the dense conditions, we propose the superiorly fine-resolved observation of CTB 37A with Chandra.

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