A Silent Revolution in Fundamental Astrophysics

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dc.authoridEker, Zeki/0000-0003-1883-6255
dc.authoridBilir, Selcuk/0000-0003-3510-1509
dc.authoridBAKIS, VOLKAN/0000-0002-3125-9010
dc.authoridSteer, Ian/0000-0003-3716-858X
dc.contributor.authorEker, Zeki
dc.contributor.authorSoydugan, Faruk
dc.contributor.authorBakis, Volkan
dc.contributor.authorBilir, Selcuk
dc.contributor.authorSteer, Ian
dc.date.accessioned2025-01-27T20:16:50Z
dc.date.available2025-01-27T20:16:50Z
dc.date.issued2022
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractArbitrariness in the zeropoint of bolometric corrections is a paradigm that is nearly a century old and leads to two more paradigms. Bolometric corrections must always be negative, and the bolometric magnitude of a star ought to be brighter than its V magnitude. Both were considered valid before the IAU 2015 General Assembly Resolution B2, a revolutionary document that supersedes all three aforementioned paradigms. The purpose of this article is to initiate new insight into and a new understanding of the fundamental astrophysics and present new capabilities to obtain standard and more accurate stellar luminosities and gain more from accurate observations in the era after Gaia. The accuracy gained will aid in advancing stellar structure and evolution theories and also Galactic and extragalactic research, observational cosmology, and searches for dark matter and dark energy.
dc.description.sponsorshipScientific and Technological Research Council (TUBITAK) [114R072]
dc.description.sponsorshipThis work has been supported in part by the Scientific and Technological Research Council (TUBITAK) under grant number 114R072. This research has made use of NASA's Astrophysics Data System Bibliographic Services. This research made use of the VizieR and Simbad databases at the CDS, Strasbourg, France. We made use of data from the European Space Agency (ESA) mission Gaia,7 processed by the Gaia Data Processing and Analysis Consortium (DPAC).8 Funding for DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement.
dc.identifier.doi10.3847/1538-3881/ac9123
dc.identifier.issn0004-6256
dc.identifier.issn1538-3881
dc.identifier.issue5
dc.identifier.scopus2-s2.0-85140224422
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.3847/1538-3881/ac9123
dc.identifier.urihttps://hdl.handle.net/20.500.12428/21405
dc.identifier.volume164
dc.identifier.wosWOS:000867431700001
dc.identifier.wosqualityQ1
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherIop Publishing Ltd
dc.relation.ispartofAstronomical Journal
dc.relation.publicationcategoryinfo:eu-repo/semantics/openAccess
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WoS_20250125
dc.subjectBolometric Corrections
dc.subjectTransformations
dc.subjectUniverse
dc.subjectColors
dc.titleA Silent Revolution in Fundamental Astrophysics
dc.typeArticle

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