The Clusters
The structure and properties of small Pd clusters
... within the framework of DFT [45, 46], using a basis set of strictly localized numerical pseudoatomic orbitals, as implemented in the SIESTA code ...[15–17]. The exchange–correlation energy was ...
10
An improved descriptor of cluster stability: application to small carbon clusters
... atomic clusters measured in cluster beams has a rich structure that arises from a complex process of growth by atom addition and evapora- tion when the clusters become hot due to the heat of ...
6
Uncloaking globular clusters in the inner galaxy
... toward the Galactic ...map the differential extinction along their fields, and produce new, cleaner, differentially dereddened CMDs of the ...give the criteria used to define our sample of ...
45
YOUNG STELLAR CLUSTERS CONTAINING MASSIVE YOUNG STELLAR OBJECTS IN THE VVV SURVEY
... study the connections of the global properties of eight young stellar clusters projected in the Vista Variables in the Via Lactea ( VVV ) ESO Large Public Survey disk area and their ...
23
Unveiling the Dynamical State of Massive Clusters through the ICL Fraction
... In the last decades, the presence of radio halos and relics has also been associated with merging clusters ( ...in the case of massive systems, through diffusive shock acceleration ( ...in ...
18
An HST/WFPC survey of bright young clusters in M31, IV Ages and mass estimates
... ascertain the real nature of candidate M 31 clusters proposed by various authors is a daunting but necessary task to keep clus- ter catalogs as complete and clean as possible from spurious ...far the ...
25
The relation between the most massive star and its parental star cluster mass
... contribution the Weidner & Kroupa (2006) list is included, cor- rected for a few errors and significantly ...expanded. The sample of 100 both new and previously published star clusters is shown ...
19
Bright globular clusters in NGC 5128: the missing link between young massive clusters and evolved massive objects
... Globular clusters observed with UVES have V -band magni- tudes ranging from ...22 clusters. The faintest ob- served cluster had V = 19.44. The typical exposure times were 1200 s for the ...
16
Massive open star clusters using the VVV survey II Discovery of six clusters with Wolf Rayet stars
... embedded clusters (red) closer to the Galactic Centre. The first two arcs follow the spiral structure indicated by H ii regions and Cepheids, but they seem offset with respect to each ...match ...
17
Methodology for Cluster Initiatives Analysis-Edición Única
... identifying the clusters of industries in which a region has a competitive ...advantage. The method combines cluster analysis with discriminating analysis, using variables derived from economic base ...
103
Discussing a new Divisive Hierarchical Clustering algorithm
... finds the number of clusters in the data but considering that the clusters included in the dataset have different ...scales. The hierarchical structure of the ...
8
The red sequence luminosity function in galaxy clusters since z 1
... along the line of sight must also be ...red-sequence clusters in our study will have another cluster that is a significant fraction of the richness of the parent cluster projected onto their ...
10
Globular cluster systems in nearby dwarf galaxies I HST/ACS observations and dynamical properties of globular clusters at low environmental density
... younger clusters (with t 4 Gyr), they will end up on the faint end of the luminosity function at an age of 14 ...those clusters would have to have unusually low metallicities ([Fe/H] ≤ − ...
15
Population Parameters of Intermediate age Star Clusters in the Large Magellanic Cloud III Dynamical Evidence for a Range of Ages Being Responsible for Extended Main sequence Turnoffs
... of the well-studied system RY Scuti have shown ejection velocities of 30–70 km s − 1 (Smith et ...provide the material for secondary generations in star clusters, one would expect the ability ...
10
The M33 Globular Cluster System with PAndAS Data: the Last Outer Halo Cluster?
... Studying the Local Group gives us the best chance to observe the remnants of galaxy formation in detail, but M33 remains to be scrutinized in as much detail as either of its larger neigh- boring ...
12
Perfiles motivacionales durante la formación inicial del docente
... Este estudio identifica, describe y analiza distintos perfiles motivacionales de estudiantes que cursan la carrera de pedagogía en enseñanza primaria. Para crear dichos perfiles se utilizó el método de análisis de ...
22
New Galactic star clusters discovered in the VVV survey
... that the majority of stars with masses > ...understanding the forma- tion, evolution, dynamics, and destruction of star clusters gain insights into the formation, evolution, and dynamics of ...
12
On the DeltaV^bump HB parameter in Globular Clusters
... constrain the fraction of CNO-enhanced stars that could be identified as a secondary RGB ...for the CNO-enhanced population two different ages, namely, 11 and 10 Gyr (see the left and right panels of ...
9
Substituting a copper atom modifies the melting of aluminum clusters
... As the impurity occupies an internal position, the electron ex- cess is mostly accommodated at the cluster ...between the doped and pure clus- ters, but one which is systematic as it is ...
9
Understanding the elusive magnetic behavior of manganese clusters
... around the energy levels to wide them up and the zero of energy is taken at the highest occupied molecular- orbital 共HOMO兲 energy ...level. The contributions coming from the different ...
8
