We have derived Mn abundances for more than 200 stars in 19 globular clusters. In addition, Mn abundance determinations have been made for a comparable number of halo field and disk stars possessing an overlapping range of metallicities and stellar parameters. Our primary data set was comprised of high-resolution spectra previously acquired at the McDonald, Lick, and Keck Observatories. To enlarge our data pool, we acquired globular and open cluster spectra from several other investigators. Data were analyzed using synthetic spectra of the 6000{AA} Mn I triplet. Hyperfine structure parameters were included in the synthetic spectra computations.
Cone search capability for table J/AJ/131/2949/table12 (Lick-Texas Group and outside source cluster observational data)
Cone search capability for table J/AJ/131/2949/table34 (Lick-Texas Group and external data source stellar model parameters and individual [Fe/H] and [Mn/Fe] values)
