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A subset of Post-AGB (PAGB) objects are the highly luminous RV Tauri variables that show similarities to Type-II Cepheids. By using a sample of known RV Tauri stars from the Magellanic Clouds we are able to determine period luminosity relationships (
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https://explore.openaire.eu/search/publication?articleId=doi_dedup___::77f5f414635161e3563d4275e561af2c
http://arxiv.org/abs/1612.00091
http://arxiv.org/abs/1612.00091
We have commenced a detailed analysis of the known sample of Galactic post-asymptotic giant branch (PAGB) objects compiled in the Toru\'n catalogue of Szczerba et al., and present, for the first time, homogeneously derived distance determinations for
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::74673f568347dcbc256c812d8975bab3
Publikováno v:
Journal of Physics: Conference Series. 728:072013
Post-AGB (PAGB) stars are short-lived, low-intermediate mass objects transitioning from the asymptotic giant branch (AGB) to the white dwarf (WD) phase. These objects are characterised by a constant, core-mass dependent luminosity and a large infrare