Excitation and Disruption of a Giant Molecular Cloud by the Sepurnova Remnant 3C 391

Reach, W. T.; Rho, J.

dc.contributor.author	Reach, W. T.	en_US
dc.contributor.author	Rho, J.	en_US
dc.date.accessioned	2004-09-24T20:58:14Z
dc.date.available	2004-09-24T20:58:14Z
dc.date.issued	1998-05	en_US
dc.identifier.citation	Astrophysical Journal	en_US
dc.identifier.citation	USA	en_US
dc.identifier.clearanceno	98-0859	en_US
dc.identifier.uri	http://hdl.handle.net/2014/19465
dc.description.abstract	The ambient molecular gas at the distance of the remnant comprises a giant molecular cloud whose edge is closely parallel to a ridge of bright non-thermal radio continuum, which evidently delineates the blast-wave into the cloud.	en_US
dc.format.extent	1122347 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en_US
dc.subject.other	giant molecular cloud supernova remnants ISM radio 3C 391 structure radio lines	en_US
dc.title	Excitation and Disruption of a Giant Molecular Cloud by the Sepurnova Remnant 3C 391	en_US