J/AJ/127/1545      Abundance ratios of 4 stars in Pal 12          (Cohen+, 2004)

Palomar 12 as a part of the Sagittarius stream: the evidence from abundance ratios. Cohen J.G. <Astron. J., 127, 1545-1554 (2004)> =2004AJ....127.1545C 2004AJ....127.1545C
ADC_Keywords: Clusters, globular ; Abundances, peculiar Keywords: globular clusters: general - globular clusters: individual (Palomar 12) - galaxies: individual (Sagittarius dSph) - stars: abundances Abstract: We present a detailed abundance analysis for 21 elements based on high-dispersion, high spectral resolution Keck spectra for four members of the outer halo "young" Galactic globular cluster Palomar 12. All four stars show identical abundance distributions with no credible indication of any star-to-star scatter. However, the abundance ratios of the Pal 12 stars are very peculiar. Description: All spectra were obtained with HIRES at the Keck Observatory in June and August 2003. Objects: ------------------------------------------ RA (2000) DE Designation(s) ------------------------------------------ 21 46 38.8 -21 15 03 Pal 12 ------------------------------------------ File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 41 311 Equivalent Widths for Palomar 12 Stars table4.dat 67 23 Derived abundances for Palomar 12 -------------------------------------------------------------------------------- See also: J/AJ/97/1360 : BV photometry of Palomar 12 (Stetson+ 1989) Table 1: Stellar parameters for the Palomar 12 sample. ---------------------------------------------------------- Name Teff logg Vt Vmag RV K dex km/s mag km/s ---------------------------------------------------------- S1 3900 0.63 1.8 14.57 28.8 1118 4000 0.84 1.8 14.84 30.0 1128 4260 1.30 1.7 15.43 28.1 1305 4465 1.62 1.7 15.86 28.8 ---------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- Ion Ion name 6- 12 F7.2 0.1nm Lambda Wavelength in angstroms 14- 17 F4.2 eV ExPot Excitation potential 19- 24 F6.2 [---] log(gf) Logarithm of the oscillator strength 26- 28 I3 10-13m EW(S1) ? Cl* Palomar 12 HC 1 equivalent width 30- 32 I3 10-13m EW(1118) ? Cl* Palomar 12 HC 1118 equivalent width 34- 36 I3 10-13m EW(1128) ? Cl* Palomar 12 HC 1128 equivalent width 38- 40 I3 10-13m EW(1305) ? Cl* Palomar 12 HC 1305 equivalent width -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 A5 --- Ion Ion 7 A1 --- n_[X/Fe](S1) [b] b: For Fe I only, we give [Fe/H] in [X/Fe] 9- 13 F5.2 --- [X/Fe](S1) Relative abundance of Cl* Palomar 12 HC 1 15- 18 F4.2 --- e_[X/Fe](S1) ?=- error on [X/Fe] (1) 20- 22 I3 --- Nlines(S1) Number of lines 24- 28 F5.2 --- [X/Fe](1118) Relative abundance of Cl* Palomar 12 HC 1118 30- 33 F4.2 --- e_[X/Fe](1118) ?=- error on [X/Fe] (1) 35- 37 I3 --- Nlines(1118) Number of lines 39- 43 F5.2 --- [X/Fe](1128) Relative abundance of Cl* Palomar 12 HC 1128 45- 48 F4.2 --- e_[X/Fe](1128) ?=- error on [X/Fe] (1) 50- 52 I3 --- Nlines(1128) Number of lines 54- 58 F5.2 --- [X/Fe](1305) Relative abundance of Cl* Palomar 12 HC 1305 60- 63 F4.2 --- e_[X/Fe](1305) ?=- error on [X/Fe] (1) 65- 67 I3 --- Nlines(1305) Number of lines -------------------------------------------------------------------------------- Note (1): 1σ rms deviation of the set of abundances derived from each of the observed absorption lines about the mean abundance. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Vannier [CDS] 07-May-2004
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