Stellar Clusters are very useful laboratories for empirically studying stellar evolution. ... All cluster stars are at the same distance . All cluster stars have the same physical age . ... CM diagram Young Cluster In this case we see the Main Sequence fully represented. The blue dots represent massive stars with short main sequence lifetimes. ... Thus, identifying the most massive star which is still on the main sequence is an effective means of determining the age of a stellar cluster. ...

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... 2003 January 7 . Open Star Cluster M38 . ... Explanation: Open cluster M38 can be seen with binoculars toward the constellation of Auriga . M38 is considered an intermediately rich open cluster of stars, each of which is about 200 million years old. ... M38, pictured above , is found only about 2.5 degrees northwest of open cluster M36 . Loosely bound by gravity, open clusters spread out over time as they orbit the galactic center and their member stars slowly escape. ... About APOD | ...

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• Отдел Изучения Галактики и переменных звезд
• APOD: 2008 August 23 - The Matter of the Bullet Cluster
• APOD: 2006 August 24 - The Matter of the Bullet Cluster

... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: Dynamical models of multiple globular cluster populations around massive galaxies . ... Different techniques have been devised to separate multiple GC populations and perform dynamical analyses. ... Within this project, the PhD candidate will examine mock models of multiple GC populations around massive galaxies, devising `blinded' functional tests and comparing the possible sources of bias in different techniques....

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• ESO - star07
• ESO - Thesis Topic: The onset of cluster formation near young high-mass stars
• AdelePlunkettAstro

... In our numerical experiments we have mainly considered two test objects provided by R. Hanisch and characterized by different types of brightness distribution; one of the objects simulates an elliptical galaxy and the other one a star cluster with size 512 512 and 256 256 pixels, respectively. ... The best performances in the restoration of the star cluster image are provided by the R-L algorithm and the LWPOS one; they give accuracies of 6%and 5%, respectively (see Table 1). ...

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• Fundamental Parameters, Integrated Red Giant Branch Mass Loss, and Dust
• Simulation of a Distant Cluster of Normal Galaxies
• Numerical Results

... NGC1850: Star Cluster in the LMC . ... Credit: R. Gilmozzi ( STScI / ESA ) S. Ewald, ( JPL ), NASA Explanation: NGC1850 is a large cluster of stars located a mere 166,000 light-years from Earth in our neighboring galaxy the Large Magellanic Cloud (LMC). ... Yellowish stars are the main cluster stars, sun-like main sequence hydrogen burners about 50 million years old. ... Publications with keywords: star cluster - LMC - stellar evolution - star - cluster - NGC 1850 . ... The Star Clusters of NGC 1313...

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• Abell 2744: Pandoras Cluster of Galaxies
• Астронет > NGC1850: Star Cluster in the LMC
• Open Star Cluster M38

... 2001 March 11 . NGC 1818: A Young Globular Cluster . ... Explanation: Globular clusters once ruled the Milky Way . Back in the old days , back when our Galaxy first formed, perhaps thousands of globular clusters roamed our Galaxy . ... There are few, if any, young globular clusters in our Milky Way Galaxy because conditions are not ripe for more to form. ... Pictured above is a "young" globular cluster residing there: NGC 1818 . ... About APOD | ...

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• APOD: December 13, 1997 - The Coma Cluster of Galaxies
• APOD: 2000 January 4 - Galaxies Cluster Toward the Great Attractor
• APOD: May 3, 1997 - Giant Cluster Bends, Breaks Galaxy Images

... AGES Precursor Observations · Targeted the M74 ( NGC 628) group · Noise falls as t (to 200s) AGES Precursor Observations · Targeted the M74 ( NGC 628) group · Noise falls as t (to 200s) AGES Precursor Observations · Targeted the M74 ( NGC 628) group · Noise falls as t (to 200s) · Detected 5 galaxies in the group KDG 010 dw0137+1540 UGC 1171 AGES Precursor ...

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• Figures for Scattering Paper
• AGES - the Arecibo Galaxy Environment Survey
• Pulsar Highlights - A Dozen new MSPs in Globular Clusters

. F IGURE . 13. The (a) metallicity and (b) age distributions of the globular clusters of Galactic origin. Different shadings are used to show the thick-disk and old-halo clusters. The curves are Gaussian fits to the corresponding histograms. discussion in the text | privious figure | next figure .

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• Vladimir Marsakov Abstracts
• Subsystems of the Galactic halo, figures

Expansion of Backfill algorithm for increasing efficiency of supercomputer «Lomonosov» Leonekov Sergei, SRCC MSU, Lomonosov Moscow State University Zhumatiy Sergey, SRCC MSU Department of Supercomputers and Quantum Informatics SLURM SLURM is a scalable, fault-tolerant cluster manager and scheduler for large computing systems. ... Output: modified queue state after each step of external scheduling 9 New Backfill-based algorithm Standard scheduler cycle (single partition example) looks like: 1. ...

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• http://www.iki.rssi.ru/comp/2010/BK.htm
• Campaign 2, October 2000

... Archives . ... my first AAS. ... I was questioned by two attendees, acquainted before the AAS, if I can suggest them clustering methods relevant to their projects. ... classification vs. clustering or supervised learning vs. unsupervised learning : the former terms from the pairs indicate the fact that the scientist already knows types of objects in his hands. ... Tags: Classification , clustering , cosmology , spatial statistics , supervised learning , test , unsupervised learning . ...

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• The AstroStat Slog outliers
• The AstroStat Slog clustering
• The AstroStat Slog LF

... Up: Data Analysis Tools, Techniques, and Software . Previous: An Automatic Astronomical Classifier Based on Topological Neural Networks . ... Teuben, P. J., Wolfire, M. G., Pound, M. W., & Mundy, L. G. 2000, in ASP Conf. ... P. J. Teuben, M. G. Wolfire, M. W. Pound, L. G. Mundy . ... We have assembled a cluster of Intel-Pentium based PCs running Linux to compute a large set of Photodissociation Region (PDR) and Dust Continuum models. ... 2000). ... Teuben, P. J. 2000, BIMA memo (in preparation) . ...

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• AIRY: Astronomical Image Restoration in interferometrY
• An Integrated Procedure for Tree N-body Simulations: FLY and AstroMD
• Automated Globular Cluster Photometry with DASHA

... GSAOI Home . ... Science . ... Deep imaging at J , H , and K is required to identify all stellar objects, brown dwarfs, and planetary mass objects in the central region of the Orion Nebula Cluster down to masses comparable to that of Jupiter. This is required to establish the initial mass function, i.e., the number of stars of each mass that have formed, in this region of intense massive star formation. ... The fields of the GSAOI detectors are shown as four green squares in each frame. ...

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• Dougal Mackey - Conference Proceedings
• IAU Commission #34 (Interstellar Matter)
• Proposed Facility

... Description . Catalog . ... In the Catalog, we publish equatorial (ЮБ 2000 , ЮД 2000 ) and galactic (l,b) coordinates of cluster centers derived as the position of overdensity in 2MASS catalog (Koposov et al. ... Distances, color-excesses and ages are the mean-square values calculated using all available evaluations from different color-magnitude diagrams. ... There are individual pages for every cluster where all available plots and parameters are published. ... 2002). ...

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• SAI Open Star Clusters (SAI OCL) Catalog

... An automated process measures jet length away from optical position (green cross) out to red Xs, allowing robust measurements and classification To investigate the Fanaroff-Riley divide as radio jets evolve through the PD diagram, we consider environmental influences on FRI and FRII sources , and conversely study the feedback from well-constrained jets on the ICM Main Idea 100 kpc 100 kpc Classifying a sample of ...

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• http://www.mrao.cam.ac.uk/~mh475/poster.pdf
• http://www.mrao.cam.ac.uk/galevol/Mei_Cambridge13.pdf
• Abstract

... The routines implemented are CLUSTER which has 8 options for hierarchical clustering and PARTITION which carries out non--hierarchical clustering. ... The former is non--hierarchical clustering or partitioning. The latter is hierarchical clustering. Brief consideration will show that a sequence of n-1 agglomerations are needed to successively merge the two closest objects and/or clusters at each stage, so that we have a set of n (singleton) clusters, n-1 clusters, ..., 2 clusters, 1 cluster. ...

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• A 20 cm VLA survey of Abell clusters of galaxies
• Radio data
• HyperLEDA documentation: parameter: vdis

... The procedure of radiometer signal integration can be considered as a sort of reducing dimension of the initial sampling space, where the samples are the result of analog-to-digital conversion. ... The probability distribution of the signal and spikes is completely known. ... The quality of the considered algorithm could be also illustrated by Figure 2 . ... One could see the considered adaptive algorithm is preferable even by low degree of compression, because all spikes have been depressed. ...

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• Laboratory for the Stellar Magnetism Study of SAO of the RAS - Magnetic stars -
• SCORPIO: IFP Gallery

. Next: Pulse Widths Up: Integrated and single pulse Previous: Integrated and single pulse . љ . Huge variations from pulse to pulse . Integrating several 100 forms a stable profile . Integrated profiles differ widely . Basic model includes core + cone . Slice in different ways to get various profiles . љ љ . Figure 54: Integrated pulse profiles . Jon Bell . Thu Dec 19 15:15:11 GMT 1996

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• Cluster Membership
• ATNF Colloquium
• correlator:mpiscript [ATNF VLBI Wiki]

This image from the NASA/ESA Hubble Space Telescope shows NGC 6388, a dynamically middle-aged globular cluster in the Milky Way. ... A new study using Hubble data has discovered that globular clusters of the same age can have dramatically different distributions of blue straggler stars within them, suggesting that clusters can age at substantially different rates. Credit: NASA/ESA/F. Ferraro (University of Bologna) ...

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• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B3079CF19-40DF-4691-819B-5AAE82D030DC%7D
• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B4CBAD180-2693-408B-AD1D-DDE2856396E7%7D
• Could gas giants be considered stars that failed to ignite? | Astronomy.com

ATMoB "Open Cluster Observing Award " Guidelines Purpose: To promote observing among the membership of the Amateur Telescope Makers of Boston through participation in the Open Clusters Observing Awards program. Introduction: This awards program is oriented towards visually observing open clusters above magnitude 9.9. ... It turns out that a very unprejudiced and convenient method to dermine the limiting magnitude is to count the number of visible stars in certain areas on the sky. ...

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• http://www.atmob.org/about/observing/awards/files/globular_cluster_instructions_2011-02-01.pdf
• Amateur Telescope Makers of Boston ATMoB Observing Awards Program

... Dnepr launch record 17 August 2011. Cluster Launch of Dnepr LV 22 August 2013 KOMPSAT-5 Launch 21 November 2013. Dnepr Cluster Mission 2013 19 June 2014. Dnepr Cluster Mission 2014 6 November 2014. ... Mission profile SHM configuration Reliability Dnepr LV Performance Launch Sites . Baikonur Cosmodrome Yasny launch base Downloads . ... Preparations for the Dnepr cluster launch mission that will carry 6 spacecraft on-board are currently under way at Baikonur Cosmodrome. ... Dnepr LV . ...

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• RS-20 (Dnepr) Cluster Launch Mission Preparation
• KOMPSAT-5 INTEGRATION
• Spacecraft Integration with Dnepr SHM