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Empirical calibration of the λ4000 Å break

dc.contributor.authorGorgas García, Francisco Javier
dc.contributor.authorCardiel López, Nicolás
dc.contributor.authorPedraz, S.
dc.contributor.authorGonzález, J. J.
dc.date.accessioned2023-06-20T20:14:24Z
dc.date.available2023-06-20T20:14:24Z
dc.date.issued1999-10
dc.descriptionCopyright The European Southern Observatory (ESO). We thank Jesús Gallego (runs 3 and 5) and Jaime Zamorano (run 3) for carrying out the observations of some stars of the sample. We also thank Emilios Harlaftis, Martín Guerrero and Reynier Peletier, the support astronomers who performed the service time observations of runs 7, 10 and 12, respectively. We are grateful to the anonymous referee for useful suggestions. The JKT, INT and WHT are operated on the island of La Palma by the Royal Greenwich Observatory at the Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias. The Calar Alto Observatory is operated jointly by the Max-Planck-Institute für Astronomie, Heidelberg, and the Spanish Comisión Nacional de Astronomía. This research has made use of the Simbad database (operated at CDS, Strasbourg, France), the NASA’s Astrophysics Data System Article Service, and the Hipparcos Catalogue. This work was supported by the Spanish “Programa Sectorial de Promoción del Conocimiento” under grant No. PB96-610.
dc.description.abstractEmpirical fitting functions, describing the behaviour of the λ4000 Å break, D_4000, in terms of effective temperature, metallicity and surface gravity, are presented. For this purpose, the break has been measured in 392 stars from the Lick/IDS Library. We have followed a very detailed error treatment in the reduction and fitting procedures, allowing for a reliable estimation of the break uncertainties. This calibration can be easily incorporated into stellar population models to provide accurate predictions of the break amplitude for, relatively old, composite systems.
dc.description.departmentDepto. de Física de la Tierra y Astrofísica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipPrograma Sectorial de Promoción del Conocimiento (MEC)
dc.description.sponsorshipMinisterio de Cultura (MEC), España
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/36918
dc.identifier.doi10.1051/aas:1999375
dc.identifier.issn0365-0138
dc.identifier.officialurlhttp://dx.doi.org/10.1051/aas:1999375
dc.identifier.relatedurlhttp://aas.aanda.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/59918
dc.issue.number1
dc.journal.titleAstronomy & astrophysics supplement series
dc.language.isoeng
dc.page.final41
dc.page.initial29
dc.publisherEDP Sciences
dc.relation.projectIDPB96-610
dc.rights.accessRightsopen access
dc.subject.cdu52
dc.subject.keywordOld stellar populations
dc.subject.keywordEarly-type galaxies
dc.subject.keywordGalactic globular-clusters
dc.subject.keywordLine-strength indexes
dc.subject.keywordStar-formation
dc.subject.keywordElliptical galaxies
dc.subject.keywordSpectral evolution
dc.subject.keywordRadial-velocities
dc.subject.keywordGradients
dc.subject.keywordMetallicities
dc.subject.ucmAstrofísica
dc.subject.ucmAstronomía (Física)
dc.titleEmpirical calibration of the λ4000 Å break
dc.typejournal article
dc.volume.number139
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