JPL Technical Report Server

Physical structure of the proto-planetary nebula CRL618.I. optical long split spectroscopy and imaging

Show simple item record

dc.contributor.author Contreras, C. S. en_US
dc.contributor.author Sahai, R. en_US
dc.contributor.author Gil de Paz, A. en_US
dc.date.accessioned 2004-09-17
dc.date.available 2004-09-17
dc.date.issued 2002-10 en_US
dc.identifier.citation Astrophysical journal, vol. 578, pp. 269-289 en_US
dc.identifier.clearanceno 03-3090 en_US
dc.identifier.uri http://hdl.handle.net/2014/7997
dc.description.abstract In this paper we present optical long-slit spectroscopy and imaging of the protoplanetary nebula CRL 618. The optical lobes of CRL 618 consist of shock-excited gas, which emits many recombination and forbidden lines, and dust, which scatters light from the innermost regions. en_US
dc.format.extent 996732 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other circumstellar matter planetary nebulae winds en_US
dc.title Physical structure of the proto-planetary nebula CRL618.I. optical long split spectroscopy and imaging en_US


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search


Browse

My Account