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Published in 2018 at "Astronomische Nachrichten"
DOI: 10.1002/asna.201913542
Abstract: We present a high resolution detailed abundance analysis for a sample of six post-AGB candidate stars, five of them had not been studied spectroscopically in the optical region. All the analyzed objects are IRAS sources…
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Keywords:
agb star;
chemical composition;
post;
post agb ... See more keywords
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Published in 2017 at "Astronomy and Astrophysics"
DOI: 10.1051/0004-6361/201731493
Abstract: Aims. We aim at describing and understanding binary interaction processes in systems with very evolved companions. Here, we focus on understanding the origin and determining the properties of the high-velocity outflow observed in one such…
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Keywords:
disk;
jet;
agb binaries;
post agb ... See more keywords
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Published in 2020 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/staa2274
Abstract: SwSt 1 (PN G001.5-06.7) is a bright and compact planetary nebula containing a late [WC]-type central star. Previous studies suggested that the nebular and stellar lines are slowly changing with time. We studied new and…
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Keywords:
star;
central star;
planetary nebula;
post agb ... See more keywords
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Published in 2020 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/staa425
Abstract: The timescales on which astronomical dust grows remain poorly understood, with important consequences for our understanding of processes like circumstellar disk evolution and planet formation.A number of post-asymptotic giant branch stars are found to host…
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Keywords:
grain growth;
discs;
growth;
post agb ... See more keywords
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Published in 2019 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stz1967
Abstract: We performed a photometric and spectroscopic analysis of two RV Tauri stars: GK Car and GZ Nor. Both objects are surrounded by hot circumstellar dust. Their pulsation periods, derived from ASAS (All Sky Automated Survey)…
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Keywords:
luminosity;
tauri stars;
post;
post agb ... See more keywords
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Published in 2019 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stz3355
Abstract: The high-resolution ($R\sim48\,000$) optical spectrum of the B-type supergiant LS 5112, identified as the optical counterpart of the post-AGB candidate IRAS 18379-1707, is analysed. We report the detailed identifications of the observed absorption and emission…
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Keywords:
18379 1707;
iras 18379;
spectroscopy;
post agb ... See more keywords