OH 231.8+4.2 : What Lurks Inside

Details OH 231.8+4.2 : What Lurks Inside OH 231.8+4.2 : What Lurks Inside

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..313...53a&link_type=abstract

Asymmetrical Planetary Nebulae III: Winds, Structure and the Thunderbird, Proceedings of the conference held 28 July - 1 August

Astronomy and Astrophysics

Astronomy

1

Scientific paper

In this contribution I will quickly review our current knowledge on the central source of the bipolar proto-planetary nebula (pPN) OH 231.8+4.2, focusing on the possibility that the Mira variable QX Pup may have no direct relationship with the nebula. This hypothesis is based on the large displacement between the well known position of the SiO masers and the axis of symmetry of the nebula. Pros and cons of this scenario are also discussed.

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