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Astronomy and astrophysics (Berlin), ISSN 0004-6361, 2014, Volume 568, pp. A12 - 15
Journal Article
Astronomy and astrophysics (Berlin), ISSN 0004-6361, 03/2016, Volume 587, p. A101
...., without planetary nebula (PN)) H-rich post-AGB stars of spectral type O(H) that show significant RV variations... 
stars: atmospheres | stars: AGB and post-AGB | binaries: spectroscopic | stars: evolution | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Stars | Displays | Stellar evolution | Spectra | Radial velocity | Companion stars | Atmospherics | Mass transfer
Journal Article
Monthly notices of the Royal Astronomical Society, ISSN 1365-2966, 12/2018, Volume 481, Issue 3, pp. 3935 - 3952
Journal Article
Astronomy and astrophysics (Berlin), ISSN 0004-6361, 2009, Volume 501, Issue 3, pp. 1207 - 1257
.... Since these AGB stars are believed to have evolved into heavily obscured post-AGB stars and PNe, the compilation of a sample of bona fide obscured post-AGB stars and PNe is important... 
stars: AGB and post-AGB | infrared: ISM | planetary nebulae: general | stars: evolution | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Physics - Astrophysics of Galaxies
Journal Article
Astronomy and astrophysics (Berlin), ISSN 0004-6361, 2006, Volume 448, Issue 2, pp. 641 - 653
Journal Article
The Astronomical journal, ISSN 1538-3881, 06/2019, Volume 158, Issue 1, p. 2
...) stars are the only viable extended source of ionizing photons. In this work, we present the first prediction of LIER-like emission from post-AGB stars that is based on fully self-consistent models of stellar evolution and photoionization... 
Physical Sciences | Astronomy & Astrophysics | Science & Technology | Radial distribution | Galaxies | Galactic evolution | Emission analysis | Stars & galaxies | Luminosity | Photons | Stellar evolution | High temperature | Asymptotic giant branch stars | Stellar models | Emissions | Active galactic nuclei | Stellar populations | Photoionization | Emission standards | Ionization | High temperatures | Convective mixing | Astronomical models | Galaxy distribution | Diagnostic systems
Journal Article
Astronomy and astrophysics (Berlin), ISSN 0004-6361, 2013, Volume 559, pp. 1 - 17
Binary post-asymptotic giant branch (post-AGB) stars are interesting laboratories to study both the evolution of binaries as well as the structure of circumstellar disks... 
Techniques: interferometric | Circumstellar matter | ISM: jets and outflows | Stars: AGB and post-AGB | Binaries: general | Scattering | Wavelengths | Stars | Emission analysis | Spectral energy distribution | Disks | Spectra | Photometry | Interferometry | Physics - Solar and Stellar Astrophysics
Journal Article
Astronomy and astrophysics (Berlin), ISSN 1432-0746, 06/2012, Volume 542, p. A53
.... It is a highly evolved post-asymptotic giant branch (post-AGB) star of spectral type F, with a large infrared excess produced by thermal emission of circumstellar dust. Methods... 
Binaries: spectroscopic | Stars: abundances | Stars: evolution | Stars: AGB and post-AGB | Binaries: general | Stars: chemically peculiar | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Physics - Solar and Stellar Astrophysics
Journal Article