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Revista mexicana de astronomía y astrofísica
Print version ISSN 0185-1101
Abstract
PENA, Miriam; RECHY-GARCIA, Jackeline S. and GARCIA-ROJAS, Jorge. Galactic kinematics of planetary nebulae with [WC] central star. Rev. mex. astron. astrofis [online]. 2013, vol.49, n.1, pp.87-99. ISSN 0185-1101.
High resolution spectra are used to analyze the galactic kinematics and distribution of a sample of planetary nebulae with [WR] and 'wel' central star ([WR]PN and WLPN). The circular and peculiar velocities, (Vpec), of the objects were derived. The results are: (a) [WR]PNe are distributed mainly in the galactic disk and they are more concentrated in a thinner disk than WLPNe and normal PNe, which corresponds to a younger population, (b) The sample was separated in Peimbert's types, and it is found that Type I PNe have Vpec < 50 km s-1, indicating young objects. Most of the [WR]PNe are of Type II showing Vpec < 60 km s-1, although a small percentage is of Type III with larger Vpec. This shows that the Wolf-Rayet phenomenon in central stars can occur at any stellar mass and in old objects. None of our WLPNe is of Type I. Thus, [WR]PNe and WLPNe are unrelated objects.
Keywords : planetary nebulae [general]; stars [kinematics and dynamics]; stars [Wolf-Rayet].