000007457 001__ 7457
000007457 005__ 20250204101633.0
000007457 0247_ $$2DOI$$a10.48550/arXiv.2411.04887
000007457 037__ $$aSCART-2025-0088
000007457 100__ $$aFrémat, Y.
000007457 245__ $$aAstrophysical Parameters associated to Hot stars in Gaia DR3
000007457 260__ $$c2024
000007457 520__ $$aHot stars, of spectral types O-, B-, and A-, represent a small fraction of the stars observed by the Gaia satellite. Their properties and the specifications of the on-board instruments make their identification challenging. In the Gaia DR3, 12,104,577 targets have been assigned a temperature greater than 7500 K. It represents ∼2.5% of the stars having an effective temperature value in the Gaia DR3 {astrophysical_parameters} table. We review the results obtained by the Apsis modules, focusing on the effective temperature, surface gravity, interstellar extinction, and vsini parameters. 
000007457 536__ $$aCNRS/$$cCNRS/$$fCNRS
000007457 594__ $$aNO
000007457 6531_ $$astars: fundamental parameters – Galaxy: stellar content – dust, extinction – catalogs
000007457 773__ $$c59-69$$pEES2023: Proceedings of the Evry Schatzman School, eds. Babusiaux, C. and Reylé, C.$$y2024
000007457 8560_ $$fyves.fremat@ksb-orb.be
000007457 85642 $$ahttps://ui.adsabs.harvard.edu/abs/2024ees..conf...59F/abstract
000007457 85642 $$ahttps://ees2023.sciencesconf.org/resource/page/id/7
000007457 905__ $$apublished in
000007457 980__ $$aNONREF