Accurate mass-radius ratios for Hyades white dwarfs

• Verfasst von: Pasquini, Luca [VerfasserIn]
• Verfasst von: Pala, A F [VerfasserIn]
• Verfasst von: Salaris, M [VerfasserIn]
• Verfasst von: Ludwig, Hans-Günter [VerfasserIn]
• Verfasst von: Leão, I [VerfasserIn]
• Verfasst von: Weiss, A [VerfasserIn]
• Verfasst von: de Medeiros, J R [VerfasserIn]
• Titel: Accurate mass-radius ratios for Hyades white dwarfs
• Verf.angabe: L. Pasquini, A.F. Pala, M. Salaris, H.-G. Ludwig, I. Leão, A. Weiss and J.R. de Medeiros
• E-Jahr: 2023
• Jahr: July 2023
• Umfang: 9 S.
• Illustrationen: Illustrationen
• Fussnoten: Veröffentlicht: 26. April 2023 ; Gesehen am 26.07.2023
• Titel Quelle: Enthalten in: Royal Astronomical SocietyMonthly notices of the Royal Astronomical Society
• Ort Quelle: Oxford : Oxford Univ. Press, 1827
• Jahr Quelle: 2023
• Band/Heft Quelle: 522(2023), 3 vom: Juli, Seite 3710-3718
• ISSN Quelle: 1365-2966
• DOI: doi:10.1093/mnras/stad1252
• Datenträger: Online-Ressource
• Sprache: eng
• K10plus-PPN: 1853647837

Abstract

We use the ESPRESSO spectrograph at the Very Large Telescope to measure velocity shifts and gravitational redshifts of eight bona fide Hyades white dwarfs, with an accuracy better than 1.5 per cent. By comparing the gravitational redshift measurements of the mass-to-radius ratio with the same ratios derived by fitting the Gaia photometry with theoretical models, we find an agreement to better than one per cent. It is possible to reproduce the observed white dwarf cooling sequence and the trend of the mass-to-radius ratios as a function of colour using isochrones with ages between 725 and 800 Myr, tuned for the Hyades. One star, EGGR 29, consistently stands out in all diagrams, indicating that it is possibly the remnant of a blue straggler. We also computed mass-to-radius ratios from published gravities and masses, determined from spectroscopy. The comparison between photometric and spectroscopic stellar parameters reveals that spectroscopic effective temperature and gravity are systematically larger than the photometric values. Spectroscopic mass-to-radius ratios disagree with those measured from gravitational redshift, indicating the presence of systematics affecting the white dwarf parameters derived from the spectroscopic analysis.