The Gaia Catalogue of Galactic AGB Stars

Abstract

This paper describes the identification of Gaia counterparts of a sample of oxygen-rich AGB stars with OH maser emission as a first step towards the compilation of a general Gaia Catalogue of Galactic AGB stars. With this catalogue, tests of evolutionary models for the AGB star population in the solar neighbourhood will become feasible. We cross-matched AGB star candidates showing OH maser emission with Gaia DR3 using a cross-match with AllWISE and 2MASS as intermediate steps to avoid ambiguities. With the help of the Virtual Observatory, we retrieved photometric data from the near-ultraviolet to the far-infrared and built spectral energy distributions (SEDs) of the sources. The SEDs were fitted with theoretical models. The fit results, together with information from the literature, allowed us to clean the sample from non-AGB stars and to obtain bolometric fluxes for the AGB stars. Distances based on Gaia parallaxes were used to derive the stellar luminosities. We identified unique Gaia counterparts for 1487 OH masers. Of these, 1172 had an unambiguous classification as AGB stars; they make up the Gaia OH/IR star sample. Parallaxes with relative errors $<$20\% and astrometric excess noise $<$1.5 mas were available for 222 OH/IR stars. We conclude that the study of the AGB population in the solar neighbourhood is limited by the obscuration by circumstellar dust, as \G\ DR3 only provides parallaxes for a few of our candidates. The location of the OH/IR stars matches that of LPV discovered by \G\ in the (BP$-$RP; G${}_{abs}$) diagram, but the OH/IR star sample is biased towards redder colours (BP$-$RP$>$4) mag and larger amplitudes ($>$1 mag in the G-band), which are typical for periodic large-amplitude Mira variables.

arXiv commentAccepted for publication in Astronomy and Astrophysics. Data available online at http://svocats.cab.inta-csic.es/gaiaagb/

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