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2011ApJ...727....9C - Astrophys. J., 727, 9 (2011/January-3)
The unusual RR Lyrae population of NGC 6101.
COHEN R.E., SARAJEDINI A., KINEMUCHI K. and LEITON R.
Abstract (from CDS):
ab> = 0.803 days and
c > = 0.393 days, and an atypically high ratio of n(c)/n(ab + c) = 0.82. Based on our derived mean properties of the RRL, NGC 6101 is Oosterhoff type II, consistent with the cluster metallicity but intriguing with respect to its kinematics.
Abstract Copyright: ∼
Journal keyword(s): Galaxy: kinematics and dynamics - globular clusters: individual: NGC 6101 - stars: horizontal-branch - stars: variables: RR Lyrae
VizieR on-line data: <Available at CDS (J/ApJ/727/9): table2.dat table3.dat table4.dat>
Nomenclature: Table 2: Cl* NGC 6101 Saw VNN (Nos 16-22) added. Table 3: [CSK2011] NNNNN N=10811 among (Nos 1-11032).
Simbad objects: 40
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