A publishing partnership

A Spatiokinematic Study of the Planetary Nebula NGC 1514

and

© 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation C. Muthu and B. G. Anandarao 2003 AJ 126 2963 DOI 10.1086/379552

1538-3881/126/6/2963

Abstract

New spatiokinematic observations were undertaken of the planetary nebula NGC 1514 in the [O III] line at 5007 Å using an imaging Fabry-Pérot spectrometer. Our results show an inner ellipsoidal shell and polar blobs that do not conform to bipolar morphology. It is argued that the nebula is a descendant of a common envelope binary system the periodicity of which is estimated to be about 10 days, with a progenitor mass of 4.5 M.

Export citation and abstract BibTeX RIS

Please wait… references are loading.
10.1086/379552