Gas clouds in dense star clusters - A possible quasar model.
Gas clouds in dense star clusters compared with quasar properties, analyzing possible energy sources like supernova explosions, stellar collisions and star gas interaction
ENERGY SOURCE↗
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Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
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Experimental investigation of base flow field at high altitudes for configurations of four and five clustered nozzles
High altitude base flow field measurements of four and five clustered conical and contoured nozzles
CLUSTER↗
Catalog of photographic magnitudes of comparison stars in globular cluster M92
Photographic magnitudes of variable stars in globular cluster M92
ASTRONOMICAL PHOTOGRAPHY↗
Variable stars in globular cluster M92
Variable stars in globular cluster M92, and evaluation of six RR-Lyrae stars
VARIABLE STAR↗
The N-body gravitational problem and the simulation of galactic clusters
Many-body gravitational problem and galactic star cluster simulation
STAR CLUSTER↗
Collective motions in a spherical star cluster
Collective motions in spherical star cluster evolution
STAR CLUSTER↗
On the stabilization of clusters of galaxies by ionized gas.
Stabilization of clusters of galaxies by ionized gas studied for recombination radiation
IONIZED GAS↗
A statistical method for inferring the initial mass function of young clusters I: procedure
This paper presents a new method for inferring the Initial Mass Function of young clusters based on intrinsic K-band Luminosity functions (LFs).
clusters↗
Applications on high performance cluster computers: production of Mars panoramic mosaic images
This paper describes the cluster machines used for a wide variety of applications, and then discusses a image data processing application in more detail.
Mars panoramic images cluster computers↗
AGN-selected clusters as revealed by weak lensing
We discuss the results in light of the cooling flow and the merger/interaction scenarios for triggering and fuelling AGN in clusters, but find that the data do not point unambiguously to neither of the two.
galaxies clusters interactions gravitational lensi↗
On the relationship between stellar rotation and radius in young clusters
We examine the early angular momentum history of stars in young clusters. We reported based on 197 photometric periods in the Orion Flanking Fields and 83 photometric periods in the NGC 2264, that PMS stars apparently do not conserve stellar angular momentum as they evolve down their connective tracks, but instead evolve at nearly constant angular velocity.
stellar rotation angular momentum clusters stars↗
Evaluating graph theoretic clustering algorithms for reliable multicasting
In this paper, we analyze the complexities of three clustering algorithms; Lorax, k-degree, and self-adjust.
clustering algorithms complexity analysis reliable↗
PVM Support for Clusters
The latest version of PVM (3.4.3) now contains support for a PC cluster running Linux, also known as a Beowulf system. A PVM user of a computer outside the Beowulf system can add the Beowulf as a single machine.
Beowulf PVM cluster interactive supercomputing↗
An X-ray Selected Galaxy Cluster at z = 1.26 (sup 1,2)
We report the discovery of an X-ray luminous galaxy cluster at z = 1.26.
clusters galaxies x-rays formation evolution gener↗
ISOCAM 15mum Search for Distant Infrared Galaxies Lensed by Clusters
In a search for lensed infrared galaxies, ISOCAM images have been obtained toward the rich clusters Abell 2218 and Abell 2219 at 15 micro m.
Infrared Galaxies Clusters↗
Mechanical and Electrostatic Dispersion of a Polydisperse Cluster of Drops for Soot Control
A model is presented for the behavior of a polydisperse cluster of spherical evaporating drops in a cylindrical, axisymmetric inviscid vortex. The formulation accounts for drop interactions and for complete dynamic and thermodynamic coupling between drops and gas.
cluster drops dense sprays soot control polydisper↗
Distance to the Fornax Cluster Using The Hubble Space Telescope: Implications for Cosmology
Using the Hubble Space Telescope (HST), we have discovred Cepheid variables in the Fornax cluster spiral galaxy, NGC 1365.
Fornax Cluster Cosmology↗
Clustering of Emerging Flux
Observations show that newly emerging flux tends to appear on the Solar surface at sites where there is flux already. This results in clustering of solar activity. Standard dynamo theories do not predict this effect.
Flux Cluster dynamo↗