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Science 15 December 1995:
Vol. 270. no. 5243, p. 1737
DOI:

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The OH maser line emission is thought to trace shock activity associated with supernovas. Yusef-Zadeh et al. (p. 1801; see the Perspective by Fukui, p. 1771) report the detection of this emission along the interface between the remnant of a supernova in the Milky Way (G359.1-0.5) and the surrounding ring of molecular gas. Comparison of the velocities of the molecular gas and the OH maser lines implies that the shock emissions are associated with CO material at the limb of the supernova remnant.




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Science. ISSN 0036-8075 (print), 1095-9203 (online)