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VizieR Online Data Catalog: Lithium in red giant stars (Charbonnel+, 2020)

dc.contributor.authorCHARBONNEL, C.
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
hal.structure.identifierUnivers, Transport, Interfaces, Nanostructures, Atmosphère et environnement, Molécules (UMR 6213) [UTINAM]
dc.contributor.authorLAGARDE, Nadège
dc.contributor.authorJASNIEWICZ, G.
dc.contributor.authorNORTH, P. L.
dc.contributor.authorSHETRONE, M.
dc.contributor.authorKRUGLER HOLLEK, J.
dc.contributor.authorSMITH, V. V.
dc.contributor.authorSMILJANIC, R.
dc.contributor.authorPALACIOS, A.
dc.contributor.authorOTTONI, G.
dc.date.issued2019-11
dc.identifier.issn0004-6361
dc.descriptiontable1.dat 829x156 Properties of giant field stars in our sample; table2a.dat 290x60 Properties of giant fields stars observed by; Luck & Hier (2007, Cat. J/AJ/133/2464) ; table2b.dat 374x60 Properties of giant fields stars observed by; Liu et al. (2014, Cat. J/ApJ/785/94) ; table2c.dat 1734x73 Properties of giant fields stars observed by; GALAH DR2 survey ; (Buder et al., 2018MNRAS.478.4513B) ; table3.dat 21x52 Properties of Li-rich giant fields stars in; our sample ; table4a.dat 2x47 Properties of Li-rich giant fields stars observed; by Luck & Hier (2007, Cat. J/AJ/133/2464) ; table4b.dat 6x47 Properties of Li-rich giant fields stars observed; by Liu et al. (2014, Cat. J/ApJ/785/94) ;
dc.description.abstractEnThe surface Li abundance was determined for a sample of 829 giant stars with accurate Gaia parallaxes for a large subsample (810 stars) complemented with accurate Hipparcos parallaxes (19 stars). Their spectra were obtained in three ground-based observatories. Three observing runs were performed at the Observatoire de Haute Provence, from 8 September to 15 September 2003 (visitor mode), from 17 January to 19 January, 2004 (service mode), and from 16 January to 16 February, 2004, service mode). High-resolution spectra were obtained with the Aurelie spectrograph attached to the 1.52m telescope. Two observing runs were performed in visitor mode at ESO- La Silla, Chile, from 3 January to 6 January, 2004, and from 5 March to 8 March, 2004. High resolution (R~43000) echelle spectra were obtained with the FEROS spectrograph attached to the MPG/ESO 2.2m telescope. Finally, a total of 92 stars were observed at the McDonald Obser vatory with the Otto Struve Telescope using the Sandiford Cassegrain Echelle Spectrometer (SES) from August 2003 to May 2004 over the course of seven observing runs. The #9 slit (1.1"x3.5") was used to yield a two pixel resolution of 60000. (7 data files).
dc.language.isoen
dc.publisherEDP Sciences
dc.source.titleVizieR On-line Data Catalog: J/A+A/633/A34. Originally published in: 2020A&A...633A..34C
dc.subject.enStars: late-type
dc.subject.enStars: giant
dc.subject.enAbundances
dc.title.enVizieR Online Data Catalog: Lithium in red giant stars (Charbonnel+, 2020)
dc.typeAutre document
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]
bordeaux.journalAstronomy and Astrophysics - A&A
bordeaux.volume363
bordeaux.title.proceedingVizieR On-line Data Catalog: J/A+A/633/A34. Originally published in: 2020A&A...633A..34C
hal.identifierhal-03864112
hal.version1
hal.popularnon
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-03864112v1
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