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H 2–12, a Misidentified Planetary Nebula in Kepler's SNR
Published online by Cambridge University Press: 26 May 2016
Abstract
H 2–12 (PN 004.5+06.8) is classified as a true or probable planetary nebula (Acker et al. 1992). We obtained narrow-band imagery and long-slit echelle spectra from several positions across H 2–12. It is shown that H 2–12 is associated with one of the brightest condensations located at the periphery of Kepler's SNR. Thus, H 2–12 should be noted as a misclassified PN.
- Type
- Part II: Planetary Nebulae Surveys and their Distribution in Galaxies
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- Copyright © Astronomical Society of the Pacific 2003