WD J004917.14-252556.81: the most massive pulsating white dwarf

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dc.contributor.authorKilic, Mukremin
dc.contributor.authorCorsico, Alejandro H.
dc.contributor.authorMoss, Adam G.
dc.contributor.authorJewett, Gracyn
dc.contributor.authorDe Geronimo, Francisco C.
dc.contributor.authorAlthaus, Leandro G.
dc.date.accessioned2025-01-20T20:10:35Z
dc.date.available2025-01-20T20:10:35Z
dc.date.issued2023
dc.description.abstractWe present Apache Point Observatory (APO) and Gemini time-series photometry of WD J004917.14-252556.81, an ultramassive DA white dwarf with T-eff = 13 020 K and log g = 9.34. We detect variability at two significant frequencies, making J0049-2525 the most massive pulsating white dwarf currently known with M-circle dot = 1.31 M-circle dot (for a CO core) or 1.26 M-circle dot(for an ONe core). J0049-2525 does not display any of the signatures of binary mergers, there is no evidence of magnetism, large tangential velocity, or rapid rotation. Hence, it likely formed through single star evolution and is likely to have an ONe core. Evolutionary models indicate that its interior is greater than or similar to 99 per cent crystallized. Asteroseismology offers an unprecedented opportunity to probe its interior structure. However, the relatively few pulsation modes detected limit our ability to obtain robust seismic solutions. Instead, we provide several representative solutions that could explain the observed properties of this star. Extensive follow-up time-series photometry of this unique target has the potential to discover a significant number of additional pulsation modes that would help overcome the degeneracies in the asteroseismic fits, and enable us to probe the interior of an approximate to 1.3 M-circle dot crystallized white dwarf.
dc.fuente.origenWOS
dc.identifier.doi10.1093/mnras/stad1113
dc.identifier.eissn1365-2966
dc.identifier.issn0035-8711
dc.identifier.urihttps://doi.org/10.1093/mnras/stad1113
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/92082
dc.identifier.wosidWOS:000978949600016
dc.issue.numero2
dc.language.isoen
dc.pagina.final2187
dc.pagina.inicio2181
dc.revistaMonthly notices of the royal astronomical society
dc.rightsacceso restringido
dc.subjectstars: evolution - stars
dc.subjectoscillations - stars
dc.subjectvariables
dc.subjectgeneral - white dwarfs
dc.titleWD J004917.14-252556.81: the most massive pulsating white dwarf
dc.typeartículo
dc.volumen522
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
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