IIA Institutional Repository

Evolutionary Status of Selected Post-AGB Single and Binary Stars in Gaia DR3

Show simple item record

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


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search DSpace


Browse

My Account