The binary central stars of PNe with the shortest orbital period

Bibcode
2011apn5.confE.259S
Santander-Garcia, M.; Rodríguez-Gil, P.; Jones, D.; Corradi, R. L. M.; Miszalski, B.; Pyrzas, S.; Rubio-Díez, M. M.
Referencia bibliográfica

Asymmetric Planetary Nebulae 5 conference, Poster Sesssion, held in Bowness-on-Windermere, U.K., 20 - 25 June 2010, A. A. Zijlstra, F. Lykou, I. McDonald, and E. Lagadec, eds. (2011) Jodrell Bank Centre for Astrophysics

Fecha de publicación:
2011
Número de autores
7
Número de autores del IAC
3
Número de citas
6
Número de citas referidas
4
Descripción
Close binarity can play a significant role in the shaping of planetary nebulae (PNe) as the system evolves through the common-envelope phase. We present the detection of two of the shortest orbital periods among PN binary central stars. These are Hen 2-428, a bipolar PN, and V458 Vul, a recent nova surrounded by a mildly bipolar planetary nebula. The properties of the central stars of these systems, of their nebulae and their possible fate are discussed.
Tipo
Sin árbitro
Nebulosas planetarias

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