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Paper: The Nature of M 2−29
Volume: 391, Hydrogen-Deficient Stars
Page: 107
Authors: Gesicki, K.; Hajduk, M.; Zijlstra, A.A.
Abstract: The hydrogen deficient central star of the PN M2−29 exhibited an RCrB-like brightness minimum, but much longer-lasting. The nebula consists of a nearly spherical ring and a monopolar jet-like structure. The images and spectra collected by us show a surprisingly static nebula surrounding a WELS star in a binary system.
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