Stellar activity in barium stars .1. Analysis of H-lines and K-lines CA-II-lines in 10 barium stars
dc.contributor.author | Cornide Castro-Piñeiro, Manuel | |
dc.contributor.author | Fernández Figueroa, María José | |
dc.contributor.author | Castro Rubio, Elisa De | |
dc.contributor.author | Armentia, J. A. | |
dc.contributor.author | Reglero, V. | |
dc.date.accessioned | 2023-06-20T20:08:40Z | |
dc.date.available | 2023-06-20T20:08:40Z | |
dc.date.issued | 1992-04 | |
dc.description | © 1992. American Astronomical Society. The 2.2 m telescope at Calar Alto Observatory is operated by the Max-Planck Institut für Astronomie at the Centro Astronómico Hispano-Alemán. We want to express our gratitude to the staff of the Observatory for their help during the observational campaign. This work has been supported by the Spanish Comisión Interministerial de Ciencia y Tecnología. | |
dc.description.abstract | High dispersion spectra have been obtained in order to study the activity level of ten barium stars by means of the Ca II H and K emission flux, looking for a relation between barium intensity index and activity. Absolute magnitudes obtained from the Wilson-Bappu relationship disagree, in some cases, with the magnitudes computed from parallaxes, but this fact is not due to barium nature. Total emission fluxes, F(H + K) or R_HK index, plotted versus effective temperature show a distribution similar to that of cool giant stars. The asymmetry of K emission line, [F(K_2ν)/F(K_2r)], has been analyzed in relation with effective temperature, in this sense barium stars behave as expected of late-type giants with the only exception of two stars. | |
dc.description.department | Depto. de Física de la Tierra y Astrofísica | |
dc.description.faculty | Fac. de Ciencias Físicas | |
dc.description.refereed | TRUE | |
dc.description.sponsorship | Comisión Interministerial de Ciencia y Tecnología (CICYT), España | |
dc.description.sponsorship | Ministerio de Ciencia e Innovación (MICINN), España | |
dc.description.status | pub | |
dc.eprint.id | https://eprints.ucm.es/id/eprint/31365 | |
dc.identifier.doi | 10.1086/116151 | |
dc.identifier.issn | 0004-6256 | |
dc.identifier.officialurl | http://dx.doi.org/10.1086/116151 | |
dc.identifier.relatedurl | http://adsabs.harvard.edu/ | |
dc.identifier.relatedurl | http://www.aanda.org | |
dc.identifier.uri | https://hdl.handle.net/20.500.14352/59665 | |
dc.issue.number | 4 | |
dc.journal.title | Astronomical journal | |
dc.language.iso | eng | |
dc.page.final | 1380 | |
dc.page.initial | 1374 | |
dc.publisher | IOP Publishing ltd | |
dc.rights.accessRights | open access | |
dc.subject.cdu | 52 | |
dc.subject.keyword | Mass-loss | |
dc.subject.keyword | Emission | |
dc.subject.ucm | Astrofísica | |
dc.subject.ucm | Astronomía (Física) | |
dc.title | Stellar activity in barium stars .1. Analysis of H-lines and K-lines CA-II-lines in 10 barium stars | |
dc.type | journal article | |
dc.volume.number | 103 | |
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dspace.entity.type | Publication | |
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