TY - JOUR
T1 - Stellar metallicities and kinematics in a gas-rich dwarf galaxy
T2 - First calcium triplet spectroscopy of red giant branch stars in WLM
AU - Leaman, Ryan
AU - Cole, Andrew A.
AU - Venn, Kim A.
AU - Tolstoy, Eline
AU - Irwin, Mike J.
AU - Szeifert, Thomas
AU - Skillman, Evan D.
AU - McConnachie, Alan W.
PY - 2009
Y1 - 2009
N2 - We present the first determination of the radial velocities and metallicities of 78 red giant stars in the isolated dwarf irregular galaxy WLM. Observations of the calcium II triplet in these stars were made with FORS2 at the VLT-UT2 in two separated fields of view in WLM, and the [Fe/H] values were conformed to the Carretta & Gratton ([Fe/H]CG97) metallicity scale. The mean metallicity is 〈[Fe/H]〉 = -1.27 0.04dex, with a standard deviation of σ = 0.37. We find that the stars in the inner field are more metal-rich by Δ[Fe/H]=0.30 0.06dex. These results are in agreement with previous photometric studies that found a radial population gradient, as well as the expectation of higher metallicities in the central star-forming regions. Age estimates using Victoria-Regina stellar models show that the youngest stars in the sample (less than 6 Gyr) are more metal-rich by Δ[Fe/H]=0.32 0.08dex. These stars also show a lower velocity dispersion at all elliptical radii compared to the metal-poor stars. Kinematics for the whole red giant sample suggest a velocity gradient approximately half that of the gas rotation curve, with the stellar component occupying a thicker disk decoupled from the HI rotation plane. Taken together, the kinematics, metallicities, and ages in our sample suggest a young metal-rich, and kinematically cold stellar population in the central gas-rich regions of WLM, surrounded by a separate dynamically hot halo of older, metal-poor stars.
AB - We present the first determination of the radial velocities and metallicities of 78 red giant stars in the isolated dwarf irregular galaxy WLM. Observations of the calcium II triplet in these stars were made with FORS2 at the VLT-UT2 in two separated fields of view in WLM, and the [Fe/H] values were conformed to the Carretta & Gratton ([Fe/H]CG97) metallicity scale. The mean metallicity is 〈[Fe/H]〉 = -1.27 0.04dex, with a standard deviation of σ = 0.37. We find that the stars in the inner field are more metal-rich by Δ[Fe/H]=0.30 0.06dex. These results are in agreement with previous photometric studies that found a radial population gradient, as well as the expectation of higher metallicities in the central star-forming regions. Age estimates using Victoria-Regina stellar models show that the youngest stars in the sample (less than 6 Gyr) are more metal-rich by Δ[Fe/H]=0.32 0.08dex. These stars also show a lower velocity dispersion at all elliptical radii compared to the metal-poor stars. Kinematics for the whole red giant sample suggest a velocity gradient approximately half that of the gas rotation curve, with the stellar component occupying a thicker disk decoupled from the HI rotation plane. Taken together, the kinematics, metallicities, and ages in our sample suggest a young metal-rich, and kinematically cold stellar population in the central gas-rich regions of WLM, surrounded by a separate dynamically hot halo of older, metal-poor stars.
KW - Galaxies: Abundances
KW - Galaxies: Dwarf
KW - Galaxies: Evolution
KW - Galaxies: Individual (WLM)-galaxies: Kinematics and dynamics
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U2 - 10.1088/0004-637X/699/1/1
DO - 10.1088/0004-637X/699/1/1
M3 - Article
AN - SCOPUS:68049139038
SN - 0004-637X
VL - 699
SP - 1
EP - 14
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 1
ER -