A 500 pc volume-limited sample of hot subluminous stars

We present a quantitative spectroscopic and kinematic analysis of a volume-complete sample of hot subluminous stars within 500 pc of the Sun, assembled using accurate parallax measurements from the Gaia space mission Data Release 3 (DR3). In total, 3226 spectra of 253 hot subdwarf stars were analyse...

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主要な著者:	Dawson H., Dorsch M., Geier S., Munday J., Pritzkuleit M., Heber U., Mattig F., Benitez-Palacios D., Vučković M., Pelisoli I., Deshmukh K., Bhat A., Kufleitner L., Uzundag M., Schaffenroth V., Reindl N., Culpan R., Raddi R., Antunes Amaral L., Istrate A. G., Justham S., Østensen R. H., Telting J. H., Steinmetz T., Rodríguez-Segovia N., Fernandez-Schlosser P., Durán-Reyes A., Arancibia-Rojas E., Latour M., Jones G. T., O’Brien M., Sahu S., Elms A.
フォーマット:	Artigo
言語:	Inglês
出版事項:	EDP Sciences 2026-03-01
シリーズ:	Astronomy & Astrophysics
主題:	catalogs binaries: general stars: evolution hertzsprung-russell and c-m diagrams stars: statistics subdwarfs
オンライン･アクセス:	https://www.aanda.org/articles/aa/full_html/2026/03/aa58123-25/aa58123-25.html
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