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Serendipity and the SDSS: Discovery of the Largest Known Planetary Nebula on the Sky

Paul C Hewett·Michael J Irwin·Evan D Skillman·Craig B Foltz·Jon P Willis·Stephen J Warren·Nicholas A Walton
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Abstract

Investigation of spectra from the Sloan Digital Sky Survey reveals the presence of a region of ionized gas of >2 degrees diameter centered approximately at alpha = 10^h 37^m delta = -00^o 18' (J2000) (Galactic coordinates l=248, b=+48). [OIII] 4959,5007 emission is particularly strong and emission from H-alpha and [NII] 6548,6583 is also detectable over a substantial area on the sky. The combination of emission line ratios, the close to zero heliocentric radial velocity and the morphology of the structure are consistent with an identification as a very nearby planetary nebula. The proximity of the hot, DO white dwarf PG1034+001 further strengthens this interpretation. The object is: i) the largest planetary nebula on the sky, ii) certainly closer than any planetary nebula other than Sh 2--216, iii) the first to be unambiguously associated with a DO white dwarf. A parallax distance for PG1034+001 would establish whether the structure is in fact the closest, and one of the physically largest, planetary nebula known.

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Paul C Hewett, Michael J Irwin, Evan D Skillman, Craig B Foltz, Jon P Willis, Stephen J Warren, Nicholas A Walton. 2003-11-04. Serendipity and the SDSS: Discovery of the Largest Known Planetary Nebula on the Sky. https://doi.org/10.1086/381139

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