ABSOLUTE PROPER MOTIONS OF 331 OPEN CLUSTERS . ... The proper motions of stars in the fields of 331 open clusters were taken from Four-Million Star Catalog (4M-catalog) of positions and proper motions (Volchkov et al. ... The absolute proper motions for 21 young open clusters have been derived by comparison of precise relative proper motions of individual stars and their corresponding absolute proper motions. ... Sign of proper motions in RA . ... 0.0001 arcsec/yr . ... rms error in RA proper motion . ...

... We have made observations of the Perseus cluster with the Westerbork Telescope at 610 MHz. ... Several newly detected sources are identified with cluster galaxies. ... No evidence is found for the existence of the previously reported ~ 65'x25' cluster halo, 3C 84B. Key words: radio galaxies - clusters - tailed radio sources buoyancy The Perseus Cluster of galaxies is one of the most fascinating systems accessible to extragalactic astronomers. ...

... In brief: the frequency-dependent radiative transfer equation is solved for a dust under assumption of spherically-symmetric geometry for its distribution taking into account particle size distribution and quantum heating effects for the very small dust particles. ... Table: Model parameters for IRAS04296+3429. ... parameter . ... hot dust shell) . ... The best fit to the spectral energy distribution of IRAS04296 is shown by heavy solid line (see Table2 for details concerning parameters of the model...

... MAO main . ... The DRAGON globular cluster simulations: a million stars, black holes and gravitational waves . ... simulations of globular clusters with a million stars on the high-performance . ... of stars in globular clusters at unprecedented detail but also shed light into . the dark world of black holes. ... clusters of single and binary black holes. ... of a globular cluster. www.mpa-garching.mpg.de/328833/hl201603 . ... MAO/NASU, 27 Akademika Zabolotnoho St. 03680 Kyiv, Ukraine . ...

... Indeed, one alteration of orbits can be the outright ejection of a planet. When several big planets are orbiting a star under each other's influence, the system is inherently unstable. ... We know of no good reason why the smallest objects with fusion should have the same mass as the smallest objects that can form by themselves. ... 6) Mission Definition . ... I don't think this mission is impossible, and will suggest a definition in a future article in Mercury. ... Good luck! . ...

... Dr. Ravil Nazirov is the head of the workshop, and Andrew Ananjev is the secretary of the workshop. ... The workshop is used to be held in the last decade of the month, preferably on Tuesdays. ... The next session will take place October 29, 1996 . ... There is "CONPAS" mailing list which you can join to discuss issues of problem solving and to be automatically notified of important dates and decisions with respect to the coming sessions. ... Secretary of the Workshop: Andrew Ananjev . ...

Astronotes Armagh Planetarium's Stellar Blog! ... Comets and Asteroids . ... Image credit:ESO/J.Emerson/VISTA. ... However others are less pessimistic and it has even been claimed that the mysterious ?Wow! signal? received in 1977 originated from the direction M55.б? Sadly, this still unexplained pulse of radio energy originated from a location rather to the northwest of M55 so I doubt if the source was this cluster (if indeed the signal was genuinely of extraterrestrial origin). ... Mysterious Wow! ...

... Cluster Antares . ... Dual Intel Xeon 2.4 GHz, RAM 4GB, HDD 36GB + 73 GB RAID 0 массив . Сервер приложений (Linux) - IBM Intel Xeon 2.8 GHz, RAM 4 GB . Сервер приложений(Windows 2003 Server) - IBM Intel Xeon 3.2 GHz, RAM 4 GB . ... Dual dedicated connectivity: 100MBit/s + 1GBit/s. PVM 3.4.6, Atlas, MPI (MPICH2), HPL, PGI CDK (HPF) . GPU сервер "Tesla" : AMD Phenom (4 cores) + Nvidia Tesla C1060 GPU . ... Intel C++ compiler . ... Intel Cluster Toolkit Compiler Edition for Linux 3.2 . ...

... We address a question if globular clusters (GC) in a protogalaxy could for some time evolve chemically as isolated systems, enriching themselves with heavy elements produced in first supernova events that follow initial star formation. We determine both the critical mass of a protoglobular cluster that is needed to retain the ejecta of the very first supernova, and the critical energy (i.e., number of supernovae) that is needed to expel the residual gas from a cluster of a given mass. ...

... Bisnovatyi-Kogan, Gennady S.; Merafina , Marco; Vaccarelli , Maria Rosaria; Spherically Symmetric Stellar Clusters with Anisotropy and Cutoff Energy in Momentum Distribution. ... We construct numerical models of spherically symmetric Newtonian stellar clusters with anisotropic distribution functions. ... Models of spherically symmetric relativistic stellar clusters with anisotropic distribution functions in relativistic regime are described by using Maxwellian distribution function with energy...

... F,L,IRREGULARSHAPE,R=F Dec 19 2006 31 Dec 19 2006 31 Nov 22 2006 8 IC 2163 17mmT4 11mmT6 R,PL, OVAL ,NND,R=F VF,VS,EL,NND,AV,R=F Galaxy SB(rs)c pec Dec 19 2006 31 Feb 10 2005 8 IC 2165 17mmT4 Planetary Neb 3b VB,PS,R=G, NO CENTRAL STAR Dec 19 2006 31 IC 2171 17mmT4 PF,CS, OVAL ,NND,R=F Galaxy IB(s)m: Dec 19 2006 31 NGC 2204 ... OIII FILTER PB,EL,PATCH,R=E,HINT-NEBULOSITY,NO FILTER NGC 2360 19mmW 12x50 25mmPL H12-7 Open Cluster 10.4 I 3 r CL,VL,RI,PC,ST9.. ...

... 1 Figure 1: The density distribution in RґZ plane Figure 2: The luminosity distribution in RґZ plane for Maxwellian kick velocity (75 km/s) 2 Figure 3: The luminosity distribution in RґZ plane for Maxwellian kick velocity (150 km/s) n(R; Z) = nHI + 2 \Delta nH2 nH2 = n 0 \Delta exp ? \GammaZ 2 2 \Delta (70pc) 2 ? If 2kpc ? R ? 3:4kpc, then nHI = n 0 \Delta exp ? \GammaZ 2 2 \Delta (140pc \Delta R=2kpc) 2 ? ; For R ? 2kpc n(R; Z) was assumed to be constant: n(R ! ...

Общая Астрономическая Конференция > Товары для астрономов > Полезное для астрономии . Astronomy with a home Computer (Patrick Moore's Practical Astronomy Series) . ... Астрономический Online журнал . ... Лунные феномены (редкие, необычные явления) Жизнь астрономов-любителей Анонсы астрономических мероприятий Астрономические клубы Наш "Старлаб" . ...

... You will receive requested data by conventional or electronic mail according to your preference. ... AHMEDABAD ALBUQUERQUE ALERT ALMA ATA 806M ALMA ATA 3340M APATITY ATHENS BAGNERES BEIJING BEIRUT BERGEN BERKELY BRISBANE BUENOS AIRES CALGARY CAPE SHMIDT CASEY CHACALTAYA CHICAGO CHURCHILL CLIMAX COLLEGE CORDOBA DALLAS DEEP RIVER DENVER DOURBES DARMSTADT DOURBES DURHAM ELLSWORTH FREIBURG FUKUSHIMA GOOSE BAY GOTTINGEN HAFELEKAR HALEAKALA HALLE HEISS IS. ...

Computer Ephemeris for 2014 from DE200/LE200. ... Sidereal Time. ... Apparent equatorial positions. Ecliptical positions. ... Chebyshev polinomial approximation of positions. ... Position and velocity. ... Dynamical time. Sidereal time. ... Osculating elements of planetary orbits. Planetary configurations (by time). ... Fundamental ephemeris. ... Ephemeris for physical observations. ... Stars. ... All comments on Computer Ephemeris please direct to the author: charlie@mail.univ.kiev.ua ...

... Structure of Data . ... Catalog . ... In SAI OCL Catalog, we introduce our work on investigation of the Milky Way system of open star clusters. The main goal of our study is a search for new clusters using huge surveys. 168 new clusters have been already discovered by us using J,H,Ks data from 2MASS point source catalog. ... For 141 new clusters, we found their physical parameters using J,H,Ks data from 2MASS catalog and, for a number of clusters, our UBVRI CCD observational magnitudes. ...

. Andrey Kravtsov "High-Resolution Cosmological Simulations of Cluster Formation" . < FIRST ] [ PREVIOUS ] [ MAIN . Slide 17 (of 17) .

The basic problems of the Laboratory are connected with researches of dynamics of minor planets and comets. ... THE ORBIT IMPROVEMENT of minor planets from optical and radar observations, . the utilization of minor planet observations for THE DETERMINATION OF ORIENTATION OF STAR CATALOGUES and DETERMINATION OF MASSES OF MINOR PLANETS BY DYNAMICAL METHOD, . THE ESTIMATION OF COLLISION PROBABILITY of minor planets with other bodies and with each other, . ...

. These documents are provided to help troubleshoot specific facilities on site: . Generator Transfer Switch . Hot Water/Heat Boiler . Compressed Air Distribution Layout (located in Boiler Room) . Kaeser Screw Compressors . Computer Room HVAC Failure . Site-wide Compressed Air System ( .doc )

Clusters of Galaxies and Large-Scale Structure ** . ... Kopylov, A. I.; Kopylova, F. G. Structure of galaxy groups and clusters measurment of their masses . ... Kopylova, F. G.; Kopylov, A. I. Pecular motions of galaxy clusters and groups in the Hercules and Leo supercluster regions . ... Kopylova, F. G.; Kopylov, A. I. Analysis of the properties of clusters of galaxies in the region of the Ursa Major supercluste . ... Kopylova, F. G.; Kopylov, A. I. The Ursa Major Supercluster of Galaxies: II. ...