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  • {{short description|Open cluster in the constellation Carina}} {{Infobox open cluster ...
    4 KB (474 words) - 04:53, 5 April 2021
  • ...is more [[robust statistics|robust]] to [[outlier]]s and able to identify clusters having non-spherical shapes and size variances. ...g algorithms these problems exist as none of the distance measures between clusters (<math>d_{min}, d_{mean}</math>) tend to work with different cluster shapes ...
    6 KB (848 words) - 23:09, 29 April 2022
  • {{Short description|Open star cluster in the constellation Ara}} {{Infobox open cluster| ...
    6 KB (866 words) - 17:47, 25 September 2024
  • ...ere the euclidean distance may not be the best measure for determining the clusters. It is important to note that this distance metric has to match with the me ...and this is essentially the [[Euclidean distance]] between the centers of clusters ''i'' and ''j'' when ''p'' equals 2. ...
    8 KB (1,286 words) - 14:21, 10 January 2025
  • ...|volume=290|pages=412–420|date=1994|title=The cases of the "disk" globular clusters NGC 6496, NGC 6624, and NGC 6637|bibcode=1994A&A...290..412R}}</ref> ...| title=Color-magnitude diagrams for six metal-rich, low-latitude globular clusters| journal=The Astronomical Journal| volume=96| pages=588| year=1988| last1=A ...
    6 KB (757 words) - 14:40, 6 September 2024
  • ...algorithm|Swendsen-Wang algorithm]] in that it generates non-trivial spin clusters informed by the interaction states on two (or more) replicas instead of jus ...this model, there are two types of bonds that can be [[Percolation theory|open]], referred to as '''blue''' and '''red'''.<ref name=":1" /> To generate th ...
    10 KB (1,442 words) - 18:32, 19 August 2024
  • ...single vertex (if that vertex is not [[Incidence (graph)|incident]] to any open bonds). Suppose an edge is open independently with probability <math>p</math> and closed otherwise, then th ...
    13 KB (1,946 words) - 13:52, 29 January 2025
  • ...d-formation rule to the plaquettes of the lattice, such that the generated clusters are informed by the frustration profile, resulting in them being smaller th The bonds will then form [[Random cluster model|clusters]] on the lattice, on which the spins can be collectively flipped (either wi ...
    6 KB (907 words) - 18:40, 11 January 2022
  • ...lated. This is known as the ''local feature relevance'' problem: different clusters might be found in different subspaces, so a global filtering of attributes ...f attributes, it is likely that some attributes are [[correlated]]. Hence, clusters might exist in arbitrarily oriented [[affine subspace]]s. ...
    18 KB (2,435 words) - 21:48, 27 October 2024
  • ...tation]]. The update is done on a "cluster" of spin variables connected by open bond variables that are generated through a [[Percolation theory|percolatio ...cting the spins <math>\sigma_n \text{ and } \sigma_m</math>(the bond is '''open'''). These values are assigned according to the following (conditional) pro ...
    13 KB (2,075 words) - 11:38, 28 April 2024
  • .../sub>) is a random collection of non-crossing loops in a simply connected, open subset of the plane. These random collections of loops are indexed by a par ...ly constructed as the collection of outer boundaries of Brownian loop soup clusters.<ref>{{harvnb|Sheffield|Werner|2010}}</ref> ...
    5 KB (717 words) - 03:32, 20 December 2023
  • ...th>d</math> dimensions, "sausages" refer to one-dimensional arrangements, "clusters" to ''<math>d</math>''-dimensional arrangements, and "pizzas" to those with ...king (that is not also a sausage) becomes possible, and with four or more, clusters (that are not also pizzas) become possible. ...
    16 KB (2,547 words) - 06:45, 7 December 2024
  • ...received the intervention. Finally, one more measurement is made after all clusters have received the intervention.<ref>{{cite journal | vauthors = Mulfinger N ...ature three main designs employing a closed [[Cohort analysis|cohort]], an open cohort, and a continuous recruitment with short exposure.<ref>{{cite journa ...
    23 KB (3,344 words) - 09:30, 18 February 2025
  • ...enta</span>). The Figure was prepared using Jmol<ref name = Jmol >Jmol: an open-source Java viewer for chemical structures in 3D. http://www.jmol.org/</ref ...a molecular mass of 28.8 kDa, and contains the [[Iron–sulfur cluster|Fe-S clusters]]. ...
    20 KB (2,791 words) - 07:05, 23 December 2024
  • ...study's findings, but this new structure proposed a [[nickel]] ion in the "open" form and a [[zinc]] ion in the "closed" form.<ref name="Hegg mechanism ACS ...s made up of two Ni-Fe-S clusters (C-cluster), two [Fe{{sub|4}}S{{sub|4}}] clusters (B-cluster) and one [Fe{{sub|4}}S{{sub|4}}] D-cluster. The D-cluster bridge ...
    18 KB (2,567 words) - 00:48, 4 February 2025
  • ...urnal | doi = 10.1088/0004-637X/775/2/134| title = The Ages of 95 Globular Clusters as Determined Using an Improved <math>\Delta V^{HB}_{TO}</math> Method Alon ...d at the time, stars from the [[Hyades (star cluster)|Hyades]] (a nearby [[open cluster]]), and several [[moving groups]], for which the [[moving cluster m ...
    23 KB (3,294 words) - 02:42, 18 July 2024
  • |caption=The supergiant IRAS 05280–6910 in the open cluster [[NGC 1984]]. It is the bright reddened object near the centre ...R. | last3 = Zijlstra | first3 = A. A. | title = Dust-enshrouded giants in clusters in the Magellanic Clouds. | arxiv = astro-ph/0507571 | doi = 10.1051/0004-6 ...
    6 KB (783 words) - 01:49, 10 December 2024
  • ...t to fronts and [[traveling wave]]s, riddled basins, riddled bifurcations, clusters and non-unique phases. Strong coupling interactions are most well known to * Spatial bifurcation to down-flow in open flow systems. ...
    19 KB (2,556 words) - 11:44, 4 October 2024
  • {{short description|Structure found in atomic clusters and nanoparticles}} ...inning|twin]]''' is a atomic structure found in atomic [[Cluster (physics)|clusters]] and also [[nanoparticles]] with some thousands of atoms. Their atomic str ...
    31 KB (4,249 words) - 19:09, 24 January 2025
  • ...velocities of ˜55000 stars and mean radial velocities of 516 Galactic open clusters and associations ...
    8 KB (956 words) - 00:43, 23 August 2024
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