reconstruction with Fast Simulation M. Iwasaki University of Oregon At the Sitges meting: tt 6jets 4jets analysis · Charged/Neutral cluster separation with Track- cluster matching · Reconstruction performance in Energy flow analysis · B-tag effect After the meeting: · In FastMC, set the cluster position resolution determined by FullMC · Study Cluster width with FullMC · ...

We present observations at 3.6, 4.5, 5.8, 8, 24, 70, and 160 ЮМm of NGC 205, the dwarf elliptical companion of M31, obtained with the Spitzer Space Telescope. ... On the basis of our mid-/far-infrared flux density measurements alone, we derive a total dust mass estimate on the order of 3.2У?104 Msolar, mainly at a temperature of ~20 K. The gas mass associated with this component matches the predicted mass returned by the dying stars from the last burst of star formation in NGC 205 (~0.5 Gyr ago). ...

... Справочник по биполярным транзисторам . Транзисторы КТ961 - 2Т990 . ... 40-100/0.15 . ... 100-250/0.15 . ... 0.5(0.5/0.05) . ... 200 . ... 300 . ... 160/0.5 . ...

Wind Dir Wind Speed Total Vis Present State Of Rainfall Sunshine 30cm 100cm Maximum Minimum Grass Cloud Weather Ground Min 1 2 2014 966.9 2.7 2.1 180 19 7 8 2 0 5.80 0.6 5.6 7.6 7.3 0.0 -0.9 2 2 2014 993.8 3.9 2.4 160 9 3 6 2 2 1.50 4.1 5.8 7.6 8.1 1.8 0.4 3 2 2014 988.6 7.7 6.7 110 24 8 6 60 1 3.90 0.0 6.0 7.5 7.8 3.5 1.6 4 2 2014 990.4 1.7 1.2 180 2 1 6 2 1 11.50 5.7 6.2 7.5 7.2 1.1 -3.0 5 2 ...

... Выше: Исследование кривых вращения галактик, Пред.: ... Так, нами были рассмотрены зависимости Mass vs , vs , Mass vs , Mass vs Dist, vs Dist (см. ... Эти зависимости достаточно хорошо известны. ... Рисунки 20 - 21, в свою очередь, демонстрируют не фундаментальные зависимости параметров галактик от расстояния (диапазон расстояний до галактик выборки мал в космологическом масштабе), а влияние эффектов селекции. ... На рисунке 20 также виден в эффект селекции. ... Рис. 17 log(Mass) vs log( ) . ...

Statistical properties of interstellar HI clouds . ... We present the results of computation of linear diameter, density and HI mass spectra for about 5000 HI clouds, which were found by their emission at 21 cm with RATAN-600 radio telescope in the region of 180 degree -3 is not a power form, but has a maximum at n H = 20 - 60 cm -3 depending of galactic latitude. The mass spectrum in the form of M X N(log M) was obtained in the mass range of 0.6 to 2.5 X 10 4 mass of the Sun. ...

... Астронет | ... Переменные Звезды | ... Микролинзирование . ... На протяжении последних нескольких лет в рамках проекта MACHO проводятся наблюдения микролинзирования звезд Большого Магелланова Облака - спутника нашей Галактики. Эффект микролинзирования заключается в гравитационной фокусировке света звезды массивным объектом, находящимся на луче зрения между звездой и наблюдателем. ... Согласно некоторым гипотезам, линзами могут являться реликтовые черные дыры или "нейтралинные звезды". ...

... Background: massive star formation! ... Scaled up low mass star formation?! What are the initial conditions (density, temperature, kinematics) for high-mass star formation?! ... Differentiate low & high-mass star-forming filaments.! ... 0.04 pc cloud structures -> protostellar or prestellar cores, i.e., the direct progenitors of individual high-mass stars.! ... High-mass stars form preferentially in ridges, high-column density (Av > 100 mag), wide (>0.3 pc) filaments present in specific regions.! ...

Next: The Evolutionary Status of Up: No Title Previous: Massive X-ray Binaries . After 25 years of pulsar studies, a radiopulsar has been discovered in a binary system with a massive optical companion (Johnston et al. ... As shown in the very first calculations of joint evolution of NS and normal stars in binaries (Kornilov and Lipunov, 1983b[ 86 ]) a considerable fraction (maybe, the majority) of NS in binary systems having an optical companion must be at the ejector љ (E) state. ... Systems . ...

... Bojan Nikolic web pages (r. 329) . Galaxy Evolution . ... By comparing narrow band spectral line indices with recent models of simple stellar populations (SSPs) we investigate trends in the star formation history as a function of galaxy mass (velocity dispersion), density of environment and galactic radius. ... MJD of the SDSS observation of the galaxy . ... The history of star formation and mass assembly in early-type galaxies . ... Copyright 2005 -- 2016, Bojan Nikolic feedback welcome ...

In the Table below the masses of some asteroids which were determined during the last years are listed. ... The listed values were determined from observations of many test bodies by the weighted least square fit for one perturbing mass and corrections to the orbit elements of all used test bodies. ... based on the observations of 98 asteroids (including 50278) with the values of standard error of mass determination less than 3.0 10 -11 M Sun . ... Mass . ... 3) Mass 121 : 0.74 x 10 -11 M Sun ; . ...

... The RAS Meteorite Collection: State on the 1 st of June, 1999 . ... About the laboratory . ... Find 1856. One mass of 16.5 kg . ... Chondrite . ... Hammadah al Hamra 163 . ... One mass of 680 g . ... One mass of 936 g . ... Find 1996. 5 masses totaling 1280 g . ... One mass of 333 g . ... One mass of 1267 g . ... One mass of 2540 g . ... One mass of 609 g . ... One mass of 4153 g . ... One mass of 3147 g . ... One mass of about 16.3 kg . ... One mass of 1544 g . ... One mass of 1084 g . ...

... From Tx manual page 1026 (6-26) . ... 100 KW rf output into dummy load . ... 14.75-16.25 . ... 180+/-100 . ... Broadband amplifier: 90 +50/-20 Watts (70 to 140 W) . page up . ...

DIMM . ... 100 000 , 2007 ­ 2009 . ... S 0.2). ... 1 3 ) , D DIMM. s DIMM s= D r0 5/3 = 5 D 2 · l2,t , Kl,t (1 4 ) 1.0 S a 0.9 0.8 0.7 LE MTF SE MTF S a 0.6 0.5 0.4 0.3 0.2 0 1 2 3 4 5 6 5/3 7 8 9 10 s = (D/r0) . ... Smin > 0.45, Smin < 0.45, - DIMM, 7 - 8 . ... Smin > 0.45 ( ) Smin < 0.45 , . ... Smin > 0.3 7 l / 0.8 0.6 S o t 1.0 0.4 0.2 Dec Nov Oct Sep Aug Jul Jun May Apr Mar Feb Jan Dec Nov Oct Sep Aug Jul Jun May Apr Mar Feb Jan Dec Nov Oct Sep 2008 2009 . ... 8 MASS/DIMM 2007 2009 , , , , . ...

IONOSPHERIC DATA foE 0.01 MHz Station MM168 LOPARSKAYA Time: UT ——————————————————————————————————————————————————————————————————————————————————————————————————————————— ... —————————————————————————————————————————————————————————————————————————————————————————————————————————————————————— 19830101 MM168 220/ 160 / 170/ 210 / 140/ 120 / 19830102 MM168 110/ 150/ 180 / 190/ 170/ 130/ 100/ 19830103 MM168 100/ 120 / 160 / 170/ ...

Blackholes2 Forum Message . ... Photons Have Mass Also. ... Posted by Duane Eddy on October 21, 2004 14:38:35 UTC . Photons have zero rest mass, however when in motion they have a non-zero mass as does all forms of energy including charge. ... A charge is a standing wave. ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

... Бренд: Patriot, Потребляемая мощность, кВА: 3,7, Минимальное напряжение питания: 220, Максимальное напряжение питания: 220, Минимальная сила тока сварки: 20, Максимальная сила тока сварки: 160, Минимальный диаметр применяемых электродов: 2, Максимальный диаметр применяемых электродов: 4, Регулировка форсирования сварочной дуги: есть, Система предотвращения залипания электрода: есть, Вес: до 5 . Сварочные аппараты . ...

. Over the last two years, we ve developed and run a set of four astrophysics MOOCs (Massive Open Online Courses), offered for free to anyone in the world who wants to take them. Around a quarter of a million students from 180 countries have enrolled in the courses - considerably more than have graduated from the ANU science it was founded. I ll present the lessons learned from this experience.

... 6 5.5 5 4.5 5.5 6 6.5 7 7.5 8 8.5 9 -1.33 -1.34 -1.35 -1.36 -1.37 -1.38 4.5 5 5.5 6 6.5 7 7.5 8 L - [Z] 0.4 0.38 0.36 0.34 0.32 0.3 0.28 4.5 5 5.5 6 6.5 7 7.5 8 L - [Fe] 0.85 0.8 5.5 6 6.5 7 7.5 8 8.5 9 0.95 0.9 M-L 1.05 1 M - M/L 13/14 M = 106.5 Msol 0.3 [Fe/H] 0.2 OB = 2 km/s 0.3 M = 106.5 Msol OB = 8 km/s 0.3 M = 107.5 Msol OB = 8 km/s 0.3 M = 108.5 Msol OB = 8 km/s [Fe/H] 0.2 0.2 [Fe/H] 0.2 [Fe/H] 0.1 0.1 0.1 ...

Dynamics and Statistics M/M 10 4 statistics R = 0.9992 2 103 dynamics R = 0.9401 10 2 2 log(/o) -1.8 -1.7 -1.6 -1.5 -1.4 -1.3 -1.2 -1.1 -1 Comparison of results of mass estimation which is received by means of our method (dynamics) for 18 clusters of Milky Way with suspected BH with data in [2] (Safonova, Shastri, Aph. ... We considered the limits of central bodies masses for 4 clusters in our Galaxy (47 Tuc, Cen, NGC 6388, M15) and G1 Globular cluster in the Galaxy Andromeda. ...