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Astrophysical parameters associated to 'hot' stars in Gaia DR3

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arxiv 2411.04887 v1 pith:N66AEZ54 submitted 2024-11-07 astro-ph.SR astro-ph.GA

classification astro-ph.SRastro-ph.GA
keywords gaiastarsparameterstemperatureastrophysicaleffectiveapsisassigned
verification ladder T0 review T1 audit T2 compute T3 formal
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Hot stars, of spectral types O-, B-, and A-, represent a small fraction of the stars observed by the Gaia satellite. Their properties and the specifications of the on-board instruments make their identification challenging. In the Gaia DR3, 12, 104,577 targets have been assigned a temperature greater than 7500 K. It represents about 2.5 percent of the stars having an effective temperature value in the Gaia DR3 astrophysical parameters table. We review the results obtained by the Apsis modules, focusing on the effective temperature, surface gravity, interstellar extinction, and V sin i parameters.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry

    astro-ph.SR 2026-08 conditional novelty 6.0 of 10

    An ensemble analysis of 873 O/B stars shows photometric variability in >93%, pulsations in ~82%, and evidence of binarity in at least 14%, including 30 newly discovered eclipsing binaries.

  2. Unveiling the Milky Way with a Gaia DR3 census of OB-type stars within 2 kpc. I. Tracing local Galactic structure, massive star-forming regions and core-collapse supernova progenitors

    astro-ph.GA 2026-07 conditional novelty 4.0 of 10

    A Gaia DR3-based census of 105,971 OB stars within 2 kpc maps local Galactic structure and identifies over 4,200 core-collapse supernova or black hole progenitor candidates.

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