dc.contributor.author |
Parthasarathy, M |
|
dc.contributor.author |
Kounkel, Marina |
|
dc.contributor.author |
Stassun, Keivan G |
|
dc.date.accessioned |
2022-11-18T06:57:06Z |
|
dc.date.available |
2022-11-18T06:57:06Z |
|
dc.date.issued |
2022-08 |
|
dc.identifier.citation |
Research Notes of the AAS, Vol. 6, No. 8, 171 |
en_US |
dc.identifier.issn |
2515-5172 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/8086 |
|
dc.description |
Open Access |
en_US |
dc.description |
Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. |
|
dc.description.abstract |
Gaia data is helping to further understand the evolutionary status of post-AGB and related stars. In this paper we present an analysis of Gaia DR3 data of post-AGB stars and post-AGB binaries with accurate parallaxes. Gaia DR3 data of 44 post-AGB candidates are analyzed, including 16 post-AGB binary candidates. Of these, 19 stars have RUWE values >1.4. For several stars, the calculated absolute luminosities confirm that they are indeed in post-AGB evolutionary stage. We find that 12 stars have relatively lower luminosities; some of them may be post-RGB stars and some may be post-HB stars. We find that IRAS 01427+4633 (BD+46 442), IRAS 16230–3410, and IRAS 19199+3950 (HP Lyr) are evolved high velocity stars. |
en_US |
dc.language.iso |
en |
en_US |
dc.publisher |
IOP Publishing |
en_US |
dc.relation.uri |
https://doi.org/10.3847/2515-5172/ac8c46 |
|
dc.rights |
© The Author(s) 2022. |
|
dc.title |
Evolutionary Status of Selected Post-AGB Single and Binary Stars in Gaia DR3 |
en_US |
dc.type |
Article |
en_US |