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Details on Acronym: [SDH2012]
[SDH2012] (Saviane+Da Costa+Held+, 2012) Write:<<[SDH2012] NGCNNNN N NNNNN>>
<<[SDH2012] Pal7 N NNNNN>>
<<[SDH2012] Pyxis N NNNNN>>
<<[SDH2012] Rup106 N NNNNN>>
<<[SDH2012] Lynga7 N NNNNN>>
<<[SDH2012] HP1 N NNNN>>
<<[SDH2012] Terzan7 N NNNN>> N: 379 Object:RGB* (SIMBAD class: RGB* = Red Giant Branch star) Note:VLT FORS2 observations of N=28 Galactic globular clusters.
N=6 (M4 = NGC 6121, M10 = NGC 6254, M71 = NGC 6838, M15 = NGC 7078, M22 = NGC 6656, M71 = NGC 6838, NGC 6397) were already studied in Da Costa et al. (2009ApJ...705.1481D). Ref:=2012A&A...540A..27S bySAVIANE I. , DA COSTA G.S., HELD E.V., SOMMARIVA V., GULLIEUSZIK M., BARBUY B., ORTOLANI S. Astron. Astrophys., 540A, 27-27 (2012) Homogeneous metallicities and radial velocities for Galactic globular clusters. First CaT metallicities for twenty clusters. oTables 3-4: <[SDH2012] NGCNNNN N NNNNN>, <[SDH2012] Pal7 N NNNNN>, <[SDH2012] Pyxis N NNNNN>, <[SDH2012] Rup106 N NNNNN>, <[SDH2012] TerzanN N NNNNN>, <[SDH2012] HP1 N NNNNN>, <[SDH2012] Lynga N NNNNN>, N=379. =E=Catalogue in electronic form as J/A+A/540/A27 Originof the Acronym: S = Created by Simbad, the CDS Database
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