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dc.contributor.authorPérez Díez, Silvia
dc.contributor.authorPitarch Martí, África
dc.contributor.authorGiakoumaki, Anastasia
dc.contributor.authorPrieto Taboada, Nagore
dc.contributor.authorFernández Ortiz de Vallejuelo, Silvia
dc.contributor.authorMartellone, Alberta
dc.contributor.authorDe Nigris, Bruno
dc.contributor.authorOsanna, Massimo
dc.contributor.authorMadariaga Mota, Juan Manuel ORCID
dc.contributor.authorMaguregui Hernando, Maite
dc.date.accessioned2021-12-13T15:15:19Z
dc.date.available2021-12-13T15:15:19Z
dc.date.issued2021-11-24
dc.identifier.citationAnalytical Chemistry 93(48) : 15870–15877 (2021)es_ES
dc.identifier.issn0003-2700
dc.identifier.urihttp://hdl.handle.net/10810/54442
dc.description.abstractIt is widely known that the vivid hue of red cinnabar can darken or turn black. Many authors have studied this transformation, but only a few in the context of the archeological site of Pompeii. In this work, the co-occurrence of different degradation patterns associated with Pompeian cinnabar-containing fresco paintings (alone or in combination with red/yellow ocher pigments) exposed to different types of environments (pre- and post-79 AD atmosphere) is reported. Results obtained from the in situ and laboratory multianalytical methodology revealed the existence of diverse transformation products in the Pompeian cinnabar, consistent with the impact of the environment. The effect of hydrogen sulfide and sulfur dioxide emitted during the 79 AD eruption on the cinnabar transformation was also evaluated by comparing the experimental evidence found on paintings exposed and not exposed to the post-79 AD atmosphere. Our results highlight that not all the darkened areas on the Pompeian cinnabar paintings are related to the transformation of the pigment itself, as clear evidence of darkening associated with the presence of manganese and iron oxide formation (rock varnish) on fragments buried before the 79 AD eruption has also been found.es_ES
dc.description.sponsorshipThe research leading to these results has received funding from “la Caixa” Foundation (Silvia Pérez-Diez, ID 100010434, Fellowship code LCF/BQ/ES18/11670017). A.P.M. is a Serra Húnter fellow. A.P.M’s research was supported by a Beatriu de Pinós postdoctoral grant (2017 BP-A 00046) of the Government of Catalonia’s Secretariat for Universities & Research of the Ministry of Economy and Knowledge. This work has been supported by the project MADyLIN (BIA2017-87063-P) funded by the Spanish Agency for Research AEI (MINECO-FEDER/UE). The authors thank for the funding provided by University of the Basque Country through the Institutionally Sponsored Open Access.es_ES
dc.language.isoenges_ES
dc.publisherACSes_ES
dc.relationinfo:eu-repo/grantAgreement/MINECO/BIA2017-87063-Pes_ES
dc.rightsinfo:eu-repo/semantics/openAccesses_ES
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/es/*
dc.subjectcinnabar, Pompeii, Raman spectroscopy, calomel, manganese oxidees_ES
dc.subjectcinnabares_ES
dc.subjectPompeiies_ES
dc.subjectRaman spectroscopyes_ES
dc.subjectcalomeles_ES
dc.subjectmanganese oxidees_ES
dc.titleWhen Red Turns Black: Influence of the 79 AD Volcanic Eruption and Burial Environment on the Blackening/Darkening of Pompeian Cinnabares_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.rights.holder© 2021 The Authors. Published by American Chemical Society cc-byes_ES
dc.relation.publisherversionhttps://pubs.acs.org/doi/10.1021/acs.analchem.1c02420es_ES
dc.identifier.doi10.1021/acs.analchem.1c02420
dc.departamentoesQuímica analíticaes_ES
dc.departamentoeuKimika analitikoaes_ES


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© 2021 The Authors. Published by American Chemical Society cc-by
Except where otherwise noted, this item's license is described as © 2021 The Authors. Published by American Chemical Society cc-by