Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2472
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dc.contributor.authorAnantharamaiah, K.R.-
dc.contributor.authorLang, Cornelia C.-
dc.contributor.authorKassim, N.E.-
dc.contributor.authorLazio, T.J.W.-
dc.contributor.authorGoss, W.M.-
dc.date.accessioned2007-05-25T09:44:21Z-
dc.date.available2007-05-25T09:44:21Z-
dc.date.issued1999-
dc.identifier.citationASP Conference Series, 1999, Vol.186, p507en
dc.identifier.isbn1-58381-012-9-
dc.identifier.urihttp://hdl.handle.net/2289/2472-
dc.descriptionRestricted Access. The Central Parsecs of the Galaxy, ASP Conference Series, Vol. 186. Eds. Heino Falcke, Angela Cotera, Wolfgang J. Duschl, Fulvio Melia, and Marcia J. Rieke, 1999.en
dc.description.abstractWe report the discovery of a new filamentary structure, G358.85+0.47, consisting of at least three mutually parallel but bent `strands', located about 1.5̂ SW of the Sgr A complex. Unlike all the other known Galactic center filaments, G358.85+0.47 is oriented parallel to the galactic plane. Based on its appearance in a 20 cm image, we give it the name 'the Pelican' for further reference.en
dc.format.extent549524 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of the Pacificen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?1999ASPC..186..507Aen
dc.rights1999 Astronomical Society of the Pacificen
dc.titleDiscovery of a new filamentary structure G358.85+0.47 -- The Pelicanen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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