Bibcode
Jones, D.; Boffin, H. M. J.; Hibbert, J.; Steinmetz, T.; Wesson, R.; Hillwig, T. C.; Sowicka, P.; Corradi, R. L. M.; García-Rojas, J.; Rodríguez-Gil, P.; Munday, J.
Referencia bibliográfica
Contributions to the XIV.0 Scientific Meeting (virtual) of the Spanish Astronomical Society
Advertised on:
7
2020
Número de citas
0
Número de citas referidas
0
Descripción
At least 20% of PNe host a post-common-envelope central star, and theoretical considerations predict that a significant fraction of these should come from common envelopes during the RGB (as opposed to the AGB). However, only a handful of candidate post-RGB PNe are known. Here, we present the discovery of a new post-RGB binary central star - discovered as part of a concerted effort to discover and characterise binary central stars of planetary nebulae in order to further our understanding of the common-envelope phase.