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1. Astronomy HyperText Book: Stellar Evolution
... Stellar Evolution is driven entirely by the never ending battle between Pressure and Gravity . As imbalances are reached, the star is driven to find a new Energy source. ... Pressure and gravitational forces are equal, the star is stable and its core is sufficiently hot to fuse Hydrogen into Helium More about main sequence stars . ... The luminosity generated by the core fusion of Helium into Carbon is far greater than the shell luminosity associated with the fusion of Hydrogen into Helium. ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/textbook/se.html -- 4.8 Кб -- 16.12.1997
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2. Effect of sources evolution on
... 172 ] Briefly, the count rate at the detector from a source at a redshift z is . ... Figure 55 shows the ``Green functions'' for the double compact binary merging rate   evolution assuming no collapse anisotropy. ... Another way that diverse peculiarities in the - distribution induced by the sources evolution could arise is connected with a possible non-monotonic character of the star formation rate in galaxies. ... 22 ] Figure  56 shows two-dimensional cuts through the parameter space. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node98.html -- 16.9 Кб -- 29.03.1997
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3. APOD: 2007 November 7 - The Sloan Great Wall: Largest Known Structure
... 2007 November 7 . The Sloan Great Wall: Largest Known Structure? ... Explanation: What is the largest structure known? ... A grouping of galaxies known as the Sloan Great Wall was discovered in the Sloan Digital Sky Survey and is a leading candidate. The Sloan Great Wall can be seen in this digitally recast contour map of galaxies in the Two Degree Field galaxy survey. ... The labeled Sloan Great Wall spans over one billion light years, longer than any structure ever measured. ... About APOD | ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap071107.html -- 5.7 Кб -- 21.12.2007
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4. Internal Structure of Stars
... 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. ...
[ Сохраненная копия ]  Ссылки http://space.univ.kiev.ua/courses/vnutr_bud_zir_e.html -- 6.6 Кб -- 23.02.2005
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5. http://www.stsci.edu/ftp/science/goods.save/Internal/aas-posters/Jogee_aas.pdf
Structure and Evolution of Bars and Disks in the GOODS Fields Jogee, S. (STScI), Conselice, C. (CalTech), Ravindranath, S. (STScI), Shlosman, I. (Kentucky), Knapen, J. H ... Lucas, R. A. (STScI), Laine, S. (SIRTF), Hornschemeier, A. (JHU), and the GOODS Team SUMMARY · Non-axisymmetric features (such as bars and spirals ) as well as general triaxialities (such as those of the bulge and halo) drive the dynamical and secular evolution of disk ... An example fit is shown in Fig 3. ...
[ Текст ]  Ссылки http://www.stsci.edu/ftp/science/goods.save/Internal/aas-posters/Jogee_aas.pdf -- 1542.3 Кб -- 16.01.2003
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6. Laboratory for the Stellar Magnetism Study of SAO of the RAS - Magnetic stars -
... The evolution of magnetic fields in OB-type stars from the study of open clusters of different ages . ... Wade G. A. The MiMeS Project: Magnetism in Massive Stars . ... Polosukhina N., Shavrina T., Drake N., Kudryavtsev D. Smirnova M. New results of the spectral observations of CPstars in the Li I 6708? spectral region with BTA telescope of SAO RAS . ... Magnetic Stars-2010 . ... List of participants . List of reports . ... Laboratory for the Stellar Magnetism Study of SAO of the RAS . ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/lizm/conferences/2010/en/reports.html -- 11.8 Кб -- 04.02.2013
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/lizm/conferences/2010/en/reports.html -- 11.8 Кб -- 02.10.2012
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/lizm/conferences/2010/en/reports.html -- 11.8 Кб -- 02.10.2012
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7. Informational system "Evolution of RG"
The project of the informational system creation on the problem of evolution of radio galaxies, as a part of the "Big Trio" project aimed on studing of distant radio galaxies, is designed. This system allows a user to operate with simulated curves of spectral energy distributions (SED) to estimate ages and redshifts by photometry data. Authors use SEDs of several models for different types of galaxies. ... The HTTP and e-mail access is organized to this system. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/sed/ -- 4.7 Кб -- 15.07.2001
[ Сохраненная копия ]  Ссылки http://sed.sao.ru/ -- 4.7 Кб -- 15.07.2001
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8. Magnetic fields, subatomic particles, etc., traveling in different directions
... Magnetic fields, subatomic particles, etc., traveling in different directions fill the universe. Do they deflect or otherwise affect one another? If so, isnт??t the information we get from them distorted? ... Neutrino astronomy, which is still in its infancy, is attractive because neutrinos interact so weakly with matter that few of these distorting effects occur. Get instant access to subscriber content on Astronomy.com! ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/magazine/ask-astro/2011/03/when-particles-collide -- 63.4 Кб -- 10.04.2016
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9. APOD: November 30, 1999 - Henize 70: A Superbubble in the LMC
... November 30, 1999 . Henize 70: A SuperBubble In The LMC . ... Explanation: Massive stars -- upwards of tens of times the mass of the Sun - profoundly affect their galactic environment. ... It is actually a luminous "superbubble" of interstellar gas about 300 light-years in diameter, blown by winds from hot, massive stars and supernova explosions , its interior filled with tenuous hot expanding gas. ... About APOD > . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap991130.html -- 4.7 Кб -- 02.10.2012
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/aggiunta/n70_vlt_big.html -- 4.6 Кб -- 16.02.2001
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10. ESO - Research Area: STELLAR STRUCTURE AND EVOLUTION
... Science Users Information > Science Activities > Science in Garching > Research Area: STELLAR STRUCTURE AND EVOLUTION . ... Reset view all 3 per page 5 per page 10 per page Sort by Title A-Z Title Z-A Date asc Date desc Research Topics Planets and Star Formation Stellar Structure and Evolution Stellar Populations Cosmology and the Early Universe Scientific Positions Faculty Fellows Scientists Students . ... Planets and Star Formation Stellar Populations Stellar Structure and Evolution Faculty . ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/sci/activities/garching/research_area_2.html -- 102.7 Кб -- 10.04.2016
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11. http://www.izmiran.rssi.ru/~ichertok/CHAINS/ANNOUNC/remarks.htm
... 2 April 1999 . The Nobeyama Radioheliograph data show that in the microwave range, besides large-scale trans-equatorial chains (see, e.g., the May 11-15, 1993 and November 1-4, 1993 events), there are also many examples displaying large and strongly evolving "longitudinal" or "internal" chains connecting remote active regions inside an active zone in one (northern or southern) hemisphere (the August 20-September 3, 1998 event). ... Last update: 2 April 1999 . ...
[ Сохраненная копия ]  Ссылки http://www.izmiran.rssi.ru/~ichertok/CHAINS/ANNOUNC/remarks.htm -- 4.9 Кб -- 02.04.1999
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