... К К Н ХЫ Ы Д в жн Ыи ж кгайи гвЕ core Hburning shell H-burning core Heburning shell Heburning double shell burning remnant 10 M M HeF irreversible evolutionary change path only possible with mass loss path only possible with mass gain reversible path with mass gain/loss M M ec M M up 11 0 6 2 1 3 4 5 15 M M up 12 M M ec 13 M M HeF 7 0 1 2 3 4 5 6 = = = = = = = main sequence M 0.7 MO ...

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... Development of Ideas of Structure and Evolution of Stars. Integral Features of Stars, Which Determine Their Structure, Direction and Rate of Evolutuion. ... Connection between Potential and Thermal Energy of Star. ... Structure of a Main Sequence Star. Features of Massive Stars Evolution on the Main Sequence. Internal Structure of the Sun. ... White Dwarfs, Their Features. ... Evolution from the Main Sequence of Massive Stars. ... Evolution of Small Mass Stars till White Dwarfs Sequence. ...

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. Subdwarfs . Metal deficient red giants in galactic field . Red horizontal branch stars . Blue horizontal branch stars . Extended horizontal branch stars . Stars inside globular clusters . W Vir type stars . IRAS-sources identified with peculiar supergiants . RCrB type stars . Sakurai's object . peculiar supergiant FG Sge .

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... Our recent observations with the Hubble Space Telescope (August 29, 2014) led to revealing a highly isolated dwarf spheroidal galaxy KKs 3 situated at a distance of 2.12 0.07 Mpc from the Milky Way. The dSph galaxy locates on the southern sky (RA=02 h 24 m 44.4 s , Dec.= ... Over the last decade, about 30 dSph galaxies have been discovered inside the Local Group through systematic search in the vicinity of M31 and more that a dozen dSphs were discovered in the nearby group around M81. ...

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• CH Cyg
• Galaxy sector, archive 2009
• Galaxy sector, archive 2006

... There are preliminary series of photometric and radio spectral observations of the above-mentioned stars, archival data on the light curves of the stars, results of the search for OH and H 2 O maser emission in IRAS point sources that possess the IR parameters similar to Miras. ... The aim is a detailed study of the maser emission variability. ... In 1996-1997, astronomical observations of Mira Ceti-type stars (miras) were carried out in three spectral ranges: optical, infrared, and radio. ...

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... We found that 10 metal-poor globular clusters are greately distinguished for anomalously small masses on the "destruction rate-mass" plain. As it turned out, these poor clusters, situated 15 kpc farther from the Galactic centre, are somewhat younger than the bulk of the metal-poor globulars, and have anomalously red horizontal branches. ... At the same time, deficiency of distant massive clusters is noticeable with increasing distance from the galactic centre. ...

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• Globular clusters with anomalously small masses, figures
• T.Borkova, V.Marsakov, Distant globular clusters with anomalously small masses

The most up-to-date information related to atmos 3.0 are collected here due to constantly increasing interest to MASS/DIMM processing software... atmos 3.0 is still beta , so the latest version is 2.97.5 (there is also 2.98.x branch which absorbs new features) . ... M' line: . ... free seeing and its relative error . ... dimm seeing and its relative error (if dimm data are present, zeros otherwise) . ... dimm turbulence power and its relative error (if dimm data are present, zeros otherwise) . ...

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• . The . MASS . Group .
• Index of /mass/download/
• Index of /mass/download/microcodes/

... Since the reddening found for the stars in Table 13 was small, no reddening correction was attempted. ... These diamonds indicate the positions of very low mass, 3 Myr old, objects from the work of Burrows et al. ... This optical V versus R - I scheme is a very powerful method of detecting very low mass (VLM) objects. ... Because of this, young brown dwarfs are intrinsically no more difficult to observe in the optical than low mass stars at the age of Orionis. ...

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• SAO Summer Intern Program Projects, 2010
• The AstroStat Slog massive data
• dictionary

arxiv:1410.4898 PSR J1738+0333: первый миллисекундный пульсар в паре с пульсирующим белым карликом (PSR J1738+0333: The First Millisecond Pulsar + Pulsating White Dwarf Binary) . ... arxiv:1410.4250 Масса менее 15 солнечных у черной дыры в ультрамощном источнике (A mass of less than 15 solar masses for the black hole in an ultraluminous X-ray source) . ... What would a binary black hole merger look like?) ... обзор arxiv:1410.6865 Лунные ресурсы: обзор (Lunar Resources: A Review) . ...

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• http://xray.sai.msu.ru/~polar/sci_rev/1505.html
• http://xray.sai.msu.ru/~polar/sci_rev/0611.html
• Rambler Mass Media

... Authors: Spyros Basilakos (Imperial College London) . ... Title: Populating a cluster of galaxies - I. Results at z=0 . ... Title: The Merger Rate to Redshift One from Kinematic Pairs: Caltech Faint Galaxy Redshift Survey XI . ... Title: Multi-wavelength observations of an evolved galaxy group: An endpoint of galaxy merging? ... 23 matches for the search pattern galaxy merging . The URL for this page is: http://xxx.itep.ru/find/astro-ph/1/galaxy+merging/0/1/0/past,all/0/0 www-admin@xxx.lanl.gov ...

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... Основная статья: Modules for Experiments in Stellar Astrophysics pdf файл статьи . ... Volume 192, Number 1 . ... 2011 ApJS 192 3 . ... Stellar physics and evolution calculations enable a broad range of research in astrophysics. ... A one-dimensional stellar evolution module, MESAstar, combines many of the numerical and physics modules for simulations of a wide range of stellar evolution scenarios ranging from very low mass to massive stars, including advanced evolutionary phases. ...

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• White Dwarf - structure
• Springer LINK:A&A-EE: Table of Contents Volume 317 Number 1 (1997)
• Index of /ftproot/pub/rec/games/Cracks-Solutions-Cheats/Branch

Twilight observations with MASS/DIMM B. Safonov Sternberg Astronomical Institute Moscow State University Comprehensive Characterization of Astronomical Sites, 2010 B. Safonov (Moscow State University) Twilight observations with MASS/DIMM SITE 2010 1 / 17 Why observe in twilight with MASS/DIMM? ... ASM includes 3 devices sensitive to background: guider, DIMM and MASS. B. Safonov (Moscow State University) Twilight observations with MASS/DIMM SITE 2010 2 / 17 Background in guider. ...

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• http://site2010.sai.msu.ru/static/doc/OVoziakova_site2010.pdf.pdf
• http://site2010.sai.msu.ru/static/doc/ATokovinin_poster_site2010.pdf
• Methods and instruments, general issues

... МАССА И МОМЕНТ ИНЕРЦИИ ЗЕМЛИ . ... Одним из возможных объяснений разности теоретических и измеренных амплитуд нутационных членов может быть упрощенная модель Земли, состоящей из упругой мантии, жидкого внешнего и упругого твердого ядра. ... The mass and the moment of inertia of the Earth . ... The estimation of the mass and the moment of inertia of the Earth with new model of Moho surface and biased inner core has shown that our result is consistent with the common values. ... Мантия . ...

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• Фундаментальные зависимости между параметрами галактик и влияние эффектов
• Marat Abubekerov - publications list
• Астрономическое отделение. Тематический указатель к Annual Review of Astronomy

... Удивите ваших близких таким неожиданным и интересным подарком, ведь необычные подарки покоряют с первого взгляда. ' title=' Светильник подвесной MARIMI pendant nickel 5x20W 230V Massive 40655/17/10 - MassiveСветильник подвесной MARIMI pendant nickel 5x20W 230V Massive 40655/17/10' border='0' align='left' width='120' style='margin-right: 20px;' hspace='7' vspace='5'/> . ...

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• branch tape US ARMY - ASMC - ASMC Linglong Green-Max Winter Grip 205/60R16xl
• german branch tape gold - ASMC - ASMC Шорты спортивные Nike
• Коврики в салон FORD Galaxy 2007->, мв., 5 шт. (текстиль, серые) -

VARIABLE STARS, THE GALACTIC HALO AND GALAXY FORMATION C. Sterken, N. Samus and L. Szabados (Eds.) 2010 Formation Mechanisms for Spheroidal Stellar Systems O. K. Sil'chenko 1 Sternberg Astronomical Institute of the Moscow State University, Moscow, Russia Abstract. Spheroidal stellar systems on various scales include elliptical galaxies, dwarf spheroidal galaxies, and globular stellar clusters. ... The formation mechanisms of the oldest globular clusters represent a puzzle yet. ... 2009). ...

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• http://sn.sai.msu.ru/~sil/preprints/my_an.pdf

... Space Res., 12, 265, 1992 planetary magnetic dipole: Mizutani, H., et al., ... Astrobiology, 7, 167, 2007 CME induced H+ ion pick-up loss at 0.05 AU for ` Hot Jupiters ' HD209458 b Mass loss ~1011 g/s even for weak CMEs Mmax strong magn. protection in reality Exoplanet magnetospheres - importance of magnetodisk Relatively large amount of observed Hot Jupiters (27%): survival of close-in giants indicates their efficient protection against of extreme plasma and radiation conditions ...

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• Публикации

... 4 November 1994 . orbit . ... 0.0128 . ... orbit period . ... satellite mass . 1950 kg . scientific payload mass . 550 kg . ... For more information send a mail to: info@sputnik.infospace.ru . 1997-2002 SMIS IKI RAN and SRC "PLANETA" Moscow, Russia. ...

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• SPUTNIK, SST White Sea

Orbital Data and Parent Star Data for: HAT-P-2__ b . ... Planetary mass . ... Stellar mass . ... Stellar T_eff . Kelvin . ... Planetary T_eff . ... Stellar Radius . ... Measured Planetary Radius . ... T_circ (w/o core) . Gyr . NaN . T_damp (w/o core) . ... Bodenheimer, Laughlin, and Lin 2003, Astrophysical Journal, v. 592, 555-563. ... Adams and Laughlin 2006, ApJ : link . ...

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• Data for XO-3_____ b
• Data for HD17156__ b
• Data for HAT-P-6__ b

This document describes how to efficiently serve an arbitrary number of virtual hosts with Apache 1.3. ... get the server name from the Host: header UseCanonicalName Off # this log format can be split per-virtual-host based on the first field LogFormat "%V %h %l %u %t \"%r\" %s %b" vcommon CustomLog logs/access_log vcommon # include the server name in the filenames used to satisfy requests VirtualDocumentRoot /www/hosts/%0/docs VirtualScriptAlias /www/hosts/%0/cgi-bin . ...

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• Apache module mod_vhost_alias
• Name-based Virtual Hosts
• Anatoly V. Zasov

. Prague, August 16, 2006 . Present classification : Suggested: . X, XB, XF, XI, XJ, XND, AM (move to cataclysmics), X, X N, XNB (approximately corresponds to XNG, a B star orbiting a compact object), Xlm (low mass), Xhm (high mass), Xmq (microquasars). In this class, advice from experts is especially needed . X-RAY VARIABLES

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• Второй пробный вариант классификации (11 мая 2006 г
• General Catalogue of Variable Stars: classification.
• General Catalogue of Variable Stars: Variability Types