JPL Technical Report Server

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

Show simple item record

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


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search


Browse

My Account