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J/A+A/537/A83       Abunbances of 9 red giants of Pal 14       (Caliskan+, 2012)

Abundance analysis of the outer halo globular cluster Palomar 14. Caliskan S., Christlieb N., Grebel E.K. <Astron. Astrophys. 537, A83 (2012)> =2012A&A...537A..83C
ADC_Keywords: Clusters, globular ; Abundances ; Stars, giant Keywords: stars: abundances - Galaxy: halo - globular clusters: individual: Pal 14 Abstract: Chemical abundances of 25 elements, which include α-, iron peak-, and neutron-capture elements, in the outer halo globular cluster Palomar 14 have been determined for the nine red giants observed with the FLAMES/UVES spectrograph. The abundance pattern of Pal 14 is similar to the inner halo GCs, halo field stars, and GCs of recognized extragalactic origin, but differs from what is customarily found in dSphs field stars. The abundance properties of Pal 14 as well as those of the other outer halo GCs are thus compatible with an accretion origin from dSphs. The neutron-capture elements show an r-process signature. Objects: ------------------------------------------------- RA (2000) DE Designation(s) ------------------------------------------------- 16 10 59.0 +14 57 42 Pal 14 = Cl Palomar 14 ------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file stars.dat 71 9 Properties and stellar parameters of target stars tablea.dat 41 1827 Linelist for the 9 red giants targeted with FLAMES/UVES (individual equivalent widths and abundances, table A1 & A2)
See also: J/A+A/448/171 : BV photometry of 3 globular clusters (Hilker+, 2006) Byte-by-byte Description of file: stars.dat
Bytes Format Units Label Explanations
1- 2 I2 --- Seq Sequential number (<Cl* Palomar 14 H NNN> in Simbad) 4- 8 A5 --- OName Other name (1) 10- 11 I2 h RAh Right ascension (J2000) 13- 14 I2 min RAm Right ascension (J2000) 16- 20 F5.2 s RAs Right ascension (J2000) 22 A1 --- DE- Declination sign (J2000) 23- 24 I2 deg DEd Declination (J2000) 26- 27 I2 arcmin DEm Declination (J2000) 29- 32 F4.1 arcsec DEs Declination (J2000) 34- 38 F5.2 mag Vmag V magnitude 40- 46 A7 s ExpTime Exposure time (in the form NNxssss) 48- 52 F5.2 km/s RV Radial velocity 54- 55 I2 --- S/N1 Signal-to-noise ratio at 5500Å (all spectra) 57- 58 I2 --- S/N2 Signal-to-noise ratio at 6630Å (all spectra) 60- 63 I4 K Teff Effective temperature 65- 67 F3.1 [cm/s2] logg Gravity surface 69- 71 F3.1 km/s xi Microturbulent velocity ξ
Note (1): names are written as: * HHNNN from Holland & Harris, 1992AJ....103..131H, <Cl* Palomar 14 HH NNN> in Simbad, or * HVNNN for Harris & van den Bergh, 1984AJ.....89.1816H
Byte-by-byte Description of file: tablea.dat
Bytes Format Units Label Explanations
1- 2 I2 --- Seq Sequential number (<Cl* Palomar 14 H NNN> in Simbad) 4- 8 A5 --- Ion Element and ionization stage (I for neutral, II for ionized species) 10- 16 F7.2 0.1nm lambda Wavelength in Angstrom 18- 21 F4.2 eV EP Excitation Potential 23- 28 F6.2 [-] loggf log of oscillator strength 30- 34 F5.2 pm EW ? Equivalent width of Ion 35 A1 -- n_EW [syn] s when EW derived from spectral synthesis rather than equivalent width fitting 37- 41 F5.2 [Sun] Abund ? Abundance
Acknowledgements: Seyma Caliskan, scaliskan(at)lsw.uni-heidelberg.de
(End) Seyma Caliskan [LSW, GERMANY], Patricia Vannier [CDS] 21-Nov-2011
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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