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dc.contributor.authorTamura, M.
dc.contributor.authorHough, J.
dc.contributor.authorChrysostomou, A.
dc.contributor.authorItoh, Y.
dc.contributor.authorMurakawa, K.
dc.contributor.authorBailey, J.
dc.date.accessioned2009-04-21T13:44:48Z
dc.date.available2009-04-21T13:44:48Z
dc.date.issued1997
dc.identifier.citationTamura , M , Hough , J , Chrysostomou , A , Itoh , Y , Murakawa , K & Bailey , J 1997 , ' Identification of the exciting source of Herbig-Haro objects 135 and 136 ' , Monthly Notices of the Royal Astronomical Society , vol. 287 , no. 4 , pp. 894-898 .
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 153520
dc.identifier.otherPURE UUID: d54b09d9-bf2c-4b2b-8f44-8857f896fe92
dc.identifier.otherdspace: 2299/3256
dc.identifier.otherScopus: 3142521125
dc.identifier.urihttp://hdl.handle.net/2299/3256
dc.descriptionOriginal article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society [Full text of this article is not available in the UHRA]
dc.description.abstractWe have identified the exciting source of the Herbig-Haro objects HH135 and 136 by near-infrared polarimetric imaging of the associated extensive reflection nebula. The source is situated at the middle of the two Herbig-Haro objects, coincident with a luminous IRAS source, and it is responsible for the excitation of both objects, although it has been suggested that there are two independent exciting sources. The source appears to be a young stellar object (presumably a Herbig Ae/Be star) surrounded by a thick circumstellar disc and it is one of the most luminous (L~=10^4 Lsolar) exciting sources of Herbig-Haro objects.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleIdentification of the exciting source of Herbig-Haro objects 135 and 136en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.identifier.urlhttp://cdsads.u-strasbg.fr/
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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