An Extremly Oxygen-Poor Planetary Nebula In The Galactic Halo
We report results of a spectrophotometric study of SBS 1150+599A, and discus s the nature of this object basing on our data. Our study shows that SBS 1150+599A is most probably a planetary nebula located in the Galactic halo and not a cataclysmic variable as originally proposed by the authors of the Second Byurakan Survey from low resolution
Tovmassian, G. et al.
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2000