Show | Sort | Column | Constraint | Explain (UCD) |
| | recno | | Record number assigned by the VizieR team. Should Not be used for identification. (meta.record) (RECORD) |
| | Name | (char) | Star name (meta.id;meta.main) (ID_MAIN) |
| | [NaI/Fe] | [-] | NaI/Fe abundance ratio Nmax=5 (phys.abund) (PHYS_ABUND_MISC) |
| | [MgI/Fe] | [-] | MgI/Fe abundance ratio Nmax=11 (phys.abund) (PHYS_ABUND_MISC) |
| | [AlI/Fe] | [-] | AlI/Fe abundance ratio Nmax=6 (phys.abund) (PHYS_ABUND_MISC) |
| | [SiI/Fe] | [-] | SiI/Fe abundance ratio Nmax=11 (phys.abund) (PHYS_ABUND_MISC) |
| | [PI/Fe] | [-] | PI/Fe abundance ratio Nmax=2 (phys.abund) (PHYS_ABUND_MISC) |
| | [SI/Fe] | [-] | SI/Fe abundance ratio Nmax=10 (phys.abund) (PHYS_ABUND_MISC) |
| | [KI/Fe] | [-] | KI/Fe abundance ratio Nmax=2 (phys.abund) (PHYS_ABUND_MISC) |
| | [CaI/Fe] | [-] | CaI/Fe abundance ratio Nmax=11 (phys.abund) (PHYS_ABUND_MISC) |
| | [ScI/Fe] | [-] | ScI/Fe abundance ratio Nmax=2 (phys.abund) (PHYS_ABUND_MISC) |
ALL cols | | | |
| | [TiI/Fe] | [-] | TiI/Fe abundance ratio Nmax=10 (phys.abund) (PHYS_ABUND_MISC) |
| | [TiII/Fe] | [-] | TiII/Fe abundance ratio Nmax=1 (phys.abund) (PHYS_ABUND_MISC) |
| | [CrI/Fe] | [-] | CrI/Fe abundance ratio Nmax=3 (phys.abund) (PHYS_ABUND_MISC) |
| | [CoI/Fe] | [-] | CoI/Fe abundance ratio Nmax=1 (phys.abund) (PHYS_ABUND_MISC) |
| | [NiI/Fe] | [-] | NiI/Fe abundance ratio Nmax=6 (phys.abund) (PHYS_ABUND_MISC) |
| | [CeII/Fe] | [-] | CeII/Fe abundance ratio Nmax=9 (phys.abund) (PHYS_ABUND_MISC) |
| | [NdII/Fe] | [-] | (n) NdII/Fe abundance ratio Nmax=1 (phys.abund) (PHYS_ABUND_MISC) |
| | [YbII/Fe] | [-] | YbII/Fe abundance ratio Nmax=1 (phys.abund) (PHYS_ABUND_MISC) |
| | 12C/13C | | 12C/13C isotopic ratio (CO features) (phys.abund) (PHYS_ABUND_MISC) |
| | [C/Fe] | [-] | C/Fe abundance ratio (CO,CI features) (phys.abund) (PHYS_ABUND_MISC) |
| | [N/Fe] | [-] | N/Fe abundance ratio (CN features) (phys.abund) (PHYS_ABUND_MISC) |
| | [O/Fe] | [-] | O/Fe abundance ratio (OH features) (phys.abund) (PHYS_ABUND_MISC) |
ALL cols | | | |