/ftp/cats/aliases/M//MRD



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J/A+A/479/141      Iz photometry, RV and EW(Li) in IC 4665       (Manzi+, 2008)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	table1.dat table2.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+A/479/141
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drwxr-xr-x 15 cats archive 258 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 310 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 481 Dec 19 2022 .message -r--r--r-- 1 cats archive 6089 Aug 7 2008 ReadMe -rw-r--r-- 1 cats archive 617 Aug 7 2008 +footg5.gif -rw-r--r-- 1 cats archive 2298 Aug 7 2008 +footg8.gif -r--r--r-- 1 cats archive 13386 Jun 19 2008 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 1190 Mar 11 2008 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/479/141 Iz photometry, RV and EW(Li) in IC 4665 (Manzi+, 2008) ================================================================================ Detection of the lithium depletion boundary in the young open cluster IC 4665. Manzi S., Randich S., De Wit W.J., Palla F. <Astron. Astrophys., 479, 141-148 (2008)> =2008A&A...479..141M ================================================================================ ADC_Keywords: Clusters, open ; Photometry ; Radial velocities ; Equivalent widths Keywords: open clusters and associations: individual: IC 4665 - stars: low-mass, brown dwarfs - stars: pre-main-sequence - stars: abundances Abstract: The so-called lithium depletion boundary (LDB) provides a secure and independent tool for deriving the ages of young open clusters. In this context, our goal is to determine membership for a sample of 147 photometrically selected candidates of the young open cluster IC 4665 and to use confirmed members to establish an age based on the LDB. Employing the FLAMES multi-object spectrograph on VLT/UT2, we have obtained intermediate-resolution spectra of the cluster candidates. The spectra were used to measure radial velocities and to infer the presence of the LiI 670.8nm doublet and Halpha emission. Description: Target stars were selected from different sources: Prosser (1993, Cat. J/AJ/105/1441), Giampapa et al. (1998ApJ...501..624G), de Wit et al. (2006, Cat. J/A+A/448/189), and a literature search on SIMBAD.