Aims.With the ongoing AKARI infrared sky survey, of much greater sensitivity than IRAS, a wealth of post-AGB objects may be discovered. It is thus time to organize our present knowledge of known post-AGB stars in the galaxy with a view to using it to search for new post-AGB objects among AKARI sources. Methods.We searched the literature available on the NASA Astrophysics Data System up to 1 October 2006, and defined criteria for classifying sources into three categories: very likely, possible and disqualified post-AGB objects. The category of very likely post-AGB objects is made up of several classes. Results.We have created an evolutionary, on-line catalogue of Galactic post-AGB objects, to be referred to as the Toruń catal...
The post-asymptotic giant branch (post-AGB) phase is a short episode in the life of a star with mass...
We have commenced a detailed analysis of the known sample of Galactic post-AGB stars compiled in the...
Context. A sample of 27 sources, cataloged as pre-main sequence stars by the Pico dos Dias Survey (P...
International audienceAims:With the ongoing AKARI infrared sky survey, of much greater sensitivity t...
With the ongoing AKARI infrared sky survey, of much greater sensitivity than IRAS, a wealth of post-...
The detected variety in chemistry and circumstellar shell morphology of the limited sample of Galact...
In this paper a first step is made to search for hot post-AGB stars in the IRAS Point Source Catalog...
Gaia provides a unique opportunity to review distances, luminosities, as well as the overall photome...
A review is presented of the most relevant results obtained in the last few years on this rare class...
Aims. We study the optical spectral properties of a sample of stars showing far infrared colours sim...
Aims.We study the optical spectral properties of a sample of stars showing far infrared colours sim...
This paper presents the first census of Galactic post-asymptotic giant branch (post-AGB) stars in th...
Context. The detected variety in chemistry and circumstellar shell morphology of the limited sample ...
"Copyright 2010 American Institute of Physics. This article may be downloaded for personal use only....
Post-AGB stars evolve on a very fast track and hence not many are known. Their spectral properties m...
The post-asymptotic giant branch (post-AGB) phase is a short episode in the life of a star with mass...
We have commenced a detailed analysis of the known sample of Galactic post-AGB stars compiled in the...
Context. A sample of 27 sources, cataloged as pre-main sequence stars by the Pico dos Dias Survey (P...
International audienceAims:With the ongoing AKARI infrared sky survey, of much greater sensitivity t...
With the ongoing AKARI infrared sky survey, of much greater sensitivity than IRAS, a wealth of post-...
The detected variety in chemistry and circumstellar shell morphology of the limited sample of Galact...
In this paper a first step is made to search for hot post-AGB stars in the IRAS Point Source Catalog...
Gaia provides a unique opportunity to review distances, luminosities, as well as the overall photome...
A review is presented of the most relevant results obtained in the last few years on this rare class...
Aims. We study the optical spectral properties of a sample of stars showing far infrared colours sim...
Aims.We study the optical spectral properties of a sample of stars showing far infrared colours sim...
This paper presents the first census of Galactic post-asymptotic giant branch (post-AGB) stars in th...
Context. The detected variety in chemistry and circumstellar shell morphology of the limited sample ...
"Copyright 2010 American Institute of Physics. This article may be downloaded for personal use only....
Post-AGB stars evolve on a very fast track and hence not many are known. Their spectral properties m...
The post-asymptotic giant branch (post-AGB) phase is a short episode in the life of a star with mass...
We have commenced a detailed analysis of the known sample of Galactic post-AGB stars compiled in the...
Context. A sample of 27 sources, cataloged as pre-main sequence stars by the Pico dos Dias Survey (P...