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J/AJ/142/63         Abundance of five stars in NGC 6397          (Koch+, 2011)

A differential chemical element analysis of the metal-poor globular cluster NGC 6397. Koch A., McWilliam A. <Astron. J., 142, 63 (2011)> =2011AJ....142...63K
ADC_Keywords: Clusters, globular ; Stars, giant ; Abundances Keywords: globular clusters: individual (NGC 6397) - stars: abundances - stars: atmospheres - stars: individual (Arcturus, Hip 66815) Abstract: We present chemical abundances in three red giants and two turnoff (TO) stars in the metal-poor Galactic globular cluster (GC) NGC 6397 based on spectroscopy obtained with the Magellan Inamori Kyocera Echelle high-resolution spectrograph on the Magellan 6.5m Clay telescope. Our results are based on a line-by-line differential abundance analysis relative to the well-studied red giant Arcturus and the Galactic halo field star HIP 66815. Description: Observations were carried out over five nights in 2005 May and June using the Magellan Inamori Kyocera Echelle spectrograph at the 6.5m Magellan2/Clay telescope. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file stars.dat 100 5 Details of observations, target properties and atmospheric parameters table2.dat 33 156 Line list for the red giants table3.dat 29 133 Line list for the turn-off stars
See also: J/A+A/287/769 : UV photometry of NGC 6397 (Burgarella+ 1994) J/PASP/108/682 : Low-Mass Stars in Outer Field in NGC 6397 (Mould+, 1996) J/A+AS/122/1 : BV photometry of variables in NGC 6397 (Kaluzny, 1997) J/AJ/119/1225 : Omega Cen and NGC 6397 Stroemgren photometry (Hughes+, 2000) J/AJ/120/3111 : Stromgren photometry of NGC 6397 (Anthony-Twarog+, 2000) J/A+A/425/509 : VI photometry of NGC 6397 (Andreuzzi+, 2004) J/A+A/490/777 : Abundances of Population II stars in NGC 6397 (Lind+, 2008) J/AJ/135/2141 : F814W+F606W photometry of NGC 6397 faint stars (Richer+, 2008) J/A+A/503/545 : Equivalent widths of Li, Na, Fe, Ca in NGC 6397 (Lind+, 2009) J/A+A/505/L13 : Lithium in globular NGC 6397 (Gonzalez Hernandez+, 2009) J/ApJ/709/241 : NGC 6397 X-rays sources characterisation (Bogdanov+, 2010) Byte-by-byte Description of file: stars.dat
Bytes Format Units Label Explanations
1- 5 I5 --- ID Star number <Cl* NGC 6397 K NNNNN> in Simbad 7- 9 A3 --- Type Type (RGB or TO=turn-off) 11- 20 A10 "YYYY/MM/DD" Date Observation date 22- 26 I5 s tExp Exposure time 28- 30 I3 pix-1 S/N Signal-to-noise ratio 32- 33 I2 h RAh Right ascension (J2000) 35- 36 I2 min RAm Right ascension (J2000) 38- 41 F4.1 s RAs Right ascension (J2000) 43 A1 --- DE- Declination sign (J2000) 44- 45 I2 deg DEd Declination (J2000) 47- 48 I2 arcmin DEm Declination (J2000) 50- 53 F4.1 arcsec DEs Declination (J2000) 55- 59 F5.2 mag Vmag V magnitude 61- 64 F4.2 mag B-V B-V colour index 66- 69 F4.2 mag V-K V-K colour index 71- 74 F4.1 km/s HV Heliocentric velocity 76- 79 I4 K Teff1 Effective temperature from V-K colour index 81- 84 I4 K Teff2 Effective temperature from spectroscopy 86- 89 I4 K Teff Average effective temperature 90 A1 --- n_Teff [a] other indices used for Teff (1) 92- 95 F4.2 [cm/s2] logg Gravity surface 97-100 F4.2 km/s Vt Microturbulent velocity
Note (1): a = Average including Teff (Hα) and the other color indices.
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 5 A5 --- Ion Ion designation 7- 13 F7.2 0.1nm lambda Wavelength 15- 18 F4.2 eV ExPot Excitation potential 20- 23 F4.1 0.1pm E13414 ? Equivalent width for star #13414 (in mÅ) 25- 28 F4.1 0.1pm E8958 ? Equivalent width for star #8958 (in mÅ) 30- 33 F4.1 0.1pm E7230 ? Equivalent width for star #7230 (in mÅ)
Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 5 A5 --- Ion Ion designation 7- 13 F7.2 0.1nm lambda Wavelength 15- 18 F4.2 eV ExPot Excitation potential 20- 24 F5.1 0.1pm E13552 ? Equivalent width for star #13552 (in mÅ) 26- 29 F4.1 0.1pm E365 ? Equivalent width for star #365 (in mÅ)
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Vannier [CDS] 12-Oct-2012
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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