The rise and fall of the NaMgAl stars J/A+A/327/587 J/A+A/327/587 Abundances of 9 solar-type stars The rise and fall of the NaMgAl stars J Tomkin B Edvardsson D L Lambert B Gustafsson Astron. Astrophys. 327 587 1997 1997A&A...327..587T Abundances, peculiar Equivalent widths Stars, dwarfs Galaxy: abundances Galaxy: evolution stars: abundances stars: fundamental parameters Line identifications, measured equivalent widths and derived chemical abundances in 9 solar-type dwarf stars, which are identified by their Bright Star (HR, (Cat. <V/50>)) numbers.
HR 448HD 956201 33 42.2-07 01 27 HR 1536HD 3056204 48 35.3-05 40 14 HR 3176HD 6722808 07 45.7+21 34 58 HR 3951HD 8672810 01 02.7+31 55 47 HR 4027HD 8898610 16 28.3+28 41 01 HR 4688HD 10721312 19 30.3+28 09 31 HR 8041HD 19996021 00 33.6-04 43 42 HR 8472HD 21085522 11 47.1+56 50 15 HR 8729HD 21701422 57 27.1+20 46 04
 Stellar equivalent widths and abundances HR HR (Cat. <V/50>) number --- Element Chemical element, e.g. 'N ' or 'Fe' --- Ion 'I ': neutral atom, 'II': singly ionized atom --- Wavel Rest frame line wavelength (Angstrom) 0.1nm EW Measured equivalent width (milliA) number=1 Blank fields when no equivalent widths were measured and no abundance was derived 0.1pm Abund Derived element abundance (1) number=2 The abundances are logarithmic element abundances [X/H] relative to the Sun, see footnote 1 of the main reference [Sun] Bengt Edvardsson Uppsala Astron. Obs. Patricia Bauer CDS 1997Sep04Bengt Edvardsson <be@astro.uu.se> J_A+A_327_587.xml