The morphology and kinematics of the Fine Ring Nebula, planetary nebula Sp 1, and the shaping influence of its binary central star
Artikel i vetenskaplig tidskrift, 2012

We present the first detailed spatiokinematical analysis and modelling of the planetary nebula Shapley 1 (Sp 1), which is known to contain a close-binary central star system. Close-binary central stars have been identified as a likely source of shaping in planetary nebulae, but with little observational support to date. Deep narrow-band imaging in the light of [O III] λ5007Å suggests the presence of a large bow shock to the west of the nebula, indicating that it is undergoing the first stages of an interaction with the interstellar medium. Further narrow-band imaging in the light of Hα + [N II] λ6584Å combined with long-slit observations of the Hα emission have been used to develop a spatiokinematical model of Sp 1. The model clearly reveals Sp 1 to be a bipolar, axisymmetric structure viewed almost pole-on. The symmetry axis of the model nebula is within a few degrees of perpendicular to the orbital plane of the central binary system – strong evidence that the central close-binary system has played an important role in shaping the nebula. Sp 1 is one of the very few nebulae to have this link, between nebular symmetry axis and binary plane, shown observationally.

outflows – planetary nebulae: individual: Sp 1 – planetary nebulae: individual: PN G329.0+01.9.

binaries: close – circumstellar matter – stars: mass-loss – stars: winds

Författare

Deborah Louise Rushton

Chalmers, Tillämpad mekanik, Strömningslära

Monthly Notices of the Royal Astronomical Society

0035-8711 (ISSN) 1365-2966 (eISSN)

Vol. 420 3 2271-2279

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Transport

Ämneskategorier

Astronomi, astrofysik och kosmologi

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2017-10-06