Gaia vbroad: Spectral-line broadening and binarity

E. Hadad*, T. Mazeh, S. Faigler, A. G.A. Brown*

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

The Gaia DR3 catalogue includes line-broadening measurements (vbroad) for 3 524 677 stars. We concentrate here on the low-mass main-sequence (MS) sub-sample of the catalogue, with (GBP - GRP)0 in the range of 1 - 1.6, which includes 81 371 sources. The colour-magnitude diagram of the sample displays two distinct strips, the brighter of which is probably mostly composed of unresolved binaries, with mass ratios close to unity. We show that the suspected binary sub-sample displays a larger vbroad distribution, which we attribute to the unresolved absorption lines of the two components of each binary. A similar effect is seen in the GALAH data.

Original languageEnglish
Article numberA214
JournalAstronomy and Astrophysics
Volume693
DOIs
StatePublished - 1 Jan 2025

Funding

FundersFunder number
Gaia Data Processing and Analysis Consortium
European Space Agency
AAO Data Central
Diabetes Patient Advocacy CoalitionA2017A/18, A/2014A/25, A/2015A/19, A2019A/1, A/2015A/3, A/2015B/1, 2021, A/2017B/16, A/2013B/13, A2019A/15, A2018A/18, A/2016A/22

    Keywords

    • Astronomical databases: miscellaneous
    • Binaries: close

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