H 2-12, A Misidentified Planetary Nebula in Kepler SNR

Details H 2-12, A Misidentified Planetary Nebula in Kepler SNR H 2-12, A Misidentified Planetary Nebula in Kepler SNR

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005rmxaa..41...57r&link_type=abstract

Revista Mexicana de Astronomía y Astrofísica Vol. 41, pp. 57-60 (2005) (http://www.astroscu.unam.mx/~rmaa/)

Astronomy and Astrophysics

Astronomy

5

Hydrodynamics, Ism: Individual (H 2-12), Ism: Jets And Outflows, Ism: Planetary Nebulae, Ism: Supernova Remnants

Scientific paper

Narrow-band direct images and long-slit, echelle spectra are presented for H 2-12. This nebula has been classified as a true planetary nebula. However, the data presented here shows that this object is actually part of the brightest knots and filaments located on the western side of Kepler's supernova remnant. Therefore, H 2-12 must be noted as a misclassified planetary nebula.

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