An enormous planetary nebula surrounding the X-ray source RXJ 2117+34

Details An enormous planetary nebula surrounding the X-ray source RXJ 2117+34 An enormous planetary nebula surrounding the X-ray source RXJ 2117+34

Nov 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aj....106.1973a&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 106, no. 5, p. 1973-1977

Astronomy and Astrophysics

Astronomy

28

Galactic Nuclei, Morphology, Planetary Nebulae, Shock Waves, Spectral Emission, White Dwarf Stars, X Ray Sources, H Alpha Line, Oxygen, Rosat Mission, Stellar Spectra, Telescopes

Scientific paper

We report the discovery of a huge planetary nebula surrounding the ROSAT x-ray source RXJ 2117+34. The source corresponds to a star which is a member of the PG 1159 spectroscopic class, which are stars that have properties intermediate between planetary nebula nuclei (PNNs) and white dwarf stars. The nebula, which is detected through its (O III) and H-alpha emission, has a maximum extent of 13 arcmin. This corresponds to a linear size of 5.3 pc at the published distance of 1.4 kpc. This size is five time greater than the largest previously known planetary nebula S68, which also surround a peculiar hot PG 1159-like PN central star. The expansion age of the RXJ nebula suggests that it is very old (approximately 1.5 x 105 yr), which is much older than its central star based on its position in the HR diagram. The morphology of the (O III) emission is interesting, showing a bipolar structure in its central parts and faint linear filaments, suggestive of shocks, in its outer regions. The discovery of an evolved PN around RXJ 2117 confirms that PG 1159 stars are transition objects between PNNs and helium-rich white dwarfs.

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