Effect of magnetic activity saturation in chromospheric flux-flux relationships

dc.contributor.authorMartínez Arnáiz, R.
dc.contributor.authorLópez Santiago, J.
dc.contributor.authorCrespo Chacón, I.
dc.contributor.authorMontes Gutiérrez, David
dc.date.accessioned2023-06-20T04:12:53Z
dc.date.available2023-06-20T04:12:53Z
dc.date.issued2011-07
dc.description© 2011 The Authors Monthly Notices of the Royal Astronomical Society. © 2011 RAS. The authors acknowledge support from the Spanish Ministerio de Educación y Ciencia (currently the Ministerio de Ciencia e Innovación), under the grant FPI20061465-00592 (Programa Nacional Formación Personal Investigador) and projects AYA2008-00695 (Programa Nacional de Astronomía y Astrofísica), AstroMadrid S2009/ESP-1496. JL-S acknowledges support by the Spanish Ministerio de Ciencia e Innovación under grant AYA2008-06423-C03-03. This research has made use of the SIMBAD data base and the VizieR catalogue access tool, operated at CDS, Strasbourg, France.
dc.description.abstractWe present a homogeneous study of chromospheric and coronal flux–flux relationships using a sample of 298 late-type dwarf active stars with spectral types F to M. The chromospheric lines were observed simultaneously in each star to avoid spread as a result of long-term variability. Unlike other works, we subtract the basal chromospheric contribution in all the spectral lines studied. For the first time, we quantify the departure of dMe stars from the general relations. We show that dK and dKe stars also deviate from the general trend. Studying the flux–colour diagrams, we demonstrate that the stars deviating from the general relations are those with saturated X-ray emission and we show that these stars also present saturation in the Hα line. Using several age spectral indicators, we show that these are younger stars than those following the general relationships. The non-universality of flux–flux relationships found in this work should be taken into account when converting between fluxes in different chromospheric activity indicators.
dc.description.departmentDepto. de Física de la Tierra y Astrofísica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipMinisterio de Ciencia e Innovación (MICINN)
dc.description.sponsorshipComunidad de Madrid (CAM)
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/37797
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dc.identifier.doi10.1111/j.1365-2966.2011.18584.x
dc.identifier.issn0035-8711
dc.identifier.officialurlhttp://dx.doi.org/10.1111/j.1365-2966.2011.18584.x
dc.identifier.relatedurlhttp://mnras.oxfordjournals.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/45050
dc.issue.number3
dc.journal.titleMonthly notices of the Royal Astronomical Society
dc.language.isoeng
dc.page.final2641
dc.page.initial2629
dc.publisherWiley
dc.relation.projectIDFPI20061465-00592
dc.relation.projectIDAYA2008-00695
dc.relation.projectIDAYA2008-06423-C03-03
dc.relation.projectIDAstroMadrid (S2009/ESP-1496)
dc.rights.accessRightsopen access
dc.subject.cdu52
dc.subject.keywordLate-type stars
dc.subject.keywordMain-sequence stars
dc.subject.keywordCA-II-H
dc.subject.keywordStellar kinematic groups
dc.subject.keywordX-ray-emission
dc.subject.keywordResolution spectroscopic observations
dc.subject.keywordYoung moving groups
dc.subject.keywordDigital sky survey
dc.subject.keywordMultiwavelength optical observations
dc.subject.keywordM-type dwarfs
dc.subject.ucmAstrofísica
dc.subject.ucmAstronomía (Física)
dc.titleEffect of magnetic activity saturation in chromospheric flux-flux relationships
dc.typejournal article
dc.volume.number414
dspace.entity.typePublication
relation.isAuthorOfPublication2dfe4286-12c7-4d3a-bfda-d298a90cc8fe
relation.isAuthorOfPublication.latestForDiscovery2dfe4286-12c7-4d3a-bfda-d298a90cc8fe
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