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https://doi.org/10.1086/133009
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Cite Publication Date: Jun 1, 1992 | |
 License type: iop-standard |
ABSTRACT Inspection of a recent Burrell Schmidt objective-prism plate indicates that the emission characteristics of the well-known Perseus cluster member HD 14422=V424 Per have greatly diminished. Further, the late -B field star HD 12994 now exhibits strong Balmer emission.
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