STUDY OF BINARY CENTRAL STARS OF PLANETARY NEBULAE WITH GALEX AND COROLLARY OPTICAL SURVEYS
Planetary Nebulae (PNe) are the descendants of low- and intermediate-mass stars (0.8--8.0 M☉). The shape of the PN takes place at some point between the asymptotic giant branch (AGB) and the white dwarf (WD) stellar phases. Among the astrophysical phenomena, the PNe shows an impressive variety of complex morphologies. In fact, most of the PNe known
Marco Antonio Gómez Muñoz
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2016