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http://hubblesite.org/newscenter/archive/releases/1996/22/text/ Probing the mysterious heart of the Crab Nebula, the tattered remains of a stellar cataclysm witnessed more than 900 years ago, astronomers using NASA's Hubble Space Telescope have found that the Crab is even more dynamic than previously understood, based on a cosmic "movie" assembled from a series of Hubble observations. ... Because of this flickering, the neutron star is also called a "pulsar." ...

... We consider the astrophysical evolution of the Galaxy over large time scales, from early stages (an age of ~10 8 yrs) to the end of traditional stellar evolution (~10 11 yrs). ... In the model considered, the basic stages of Galactic evolution are as follows. ... Essentially all other basic parameters of the Galaxy vary little. ... The final "stellar epoch" in the life of the Galaxy is completed ~10 13 yrs after its formation, when the evolution of the least massive stars comes to an end. ...

... Phase light curves of binary model that consists of a primary component with mass M 1 and a secondary component with mass M 2 . ... The input parameters of the problem are the accretion rate onto the binary components ( ), the component mass ratio q = M 2 /M 1 , the orbital inclination to the line of sight , the eccentricity e, the rotation angle of the apsidal line relative to the observer , and the parameter c characterizing viscosity. ...

... Under certain conditions, like those in the nucleus of a QSO, all atoms can be made to emit light at particular wavelengths. ... If that source is approaching the observer, the wave is squashed up onto itself making the wavelength shorter. ... This is redshift. ... You can see how the section of the QSO spectrum which we observe changes with redshift. ... We then see how far we had to slide the observed spectrum along the scale to make it match and that is the objects redshift. ... The 2QZ team . ...

... Tracy Caldwell Dyson (Ph.D.) . NASA Astronaut . ... Caldwell Dyson has worked inside the Mission Control Center as spacecraft communicator (CAPCOM) for both space shuttle and space station operations, serving also as the lead CAPCOM for ISS Increment 11. ... Caldwell Dyson operated EndeavourтАЩs robotic arm to maneuver the Orbiter Boom Sensor System (OBSS) and handover the S5 truss segment to the space station, and served as the intravehicular (IV) crew member, directing the four spacewalks. ...

... MASTER Net is 56 square degrees per 1 exposition . ... 06 Dec 2015: GRB 151205B: MASTER-NET early optical observations GCN18665 . ... 18 Nov 2015: GRB 151118A: MASTER-NET optical observations GCN18613 . ... 12 Nov 2015: GRB 151112A: MASTER-NET optical limit GCN18591 . ... 07 Nov 2015: GRB 151107A: MASTER-NET optical observations GCN18565 . ... 31 Oct 2015: Five OTs detected by Global Robotic MASTER Net ATel8232 . ... 02 Oct 2015: GRB 151001B: MASTER-NET early optical observations GCN18380 . ...

... Samara State Aerospace University Students life Student clubs . Samara State Aerospace University provides a large number of students associations, clubs, sections and project groups. ... There is student press center at Samara State Aerospace University which includes: Kakovkin Illuminator photo club, Bort 3 video log, a journalists club and a students' radio station. ... Samara State Aerospace University also runs a students' volunteer center. ... Sputnik International Student Club . ...

... Author(s) : Nikolai G. Bochkarev . Pages : 0 to 0 . ... A study of thin disk with radial flow for perfect fluid disk in Kerr geometry . ... The present stellar populations and the origin of galaxies . ... Stellar subsystems of edge-on disk galaxies . ... Properties and Structural Features of Early-Type Disk Galaxies with Multi-Tier Disks . ... and LSB galaxies . ... Galactic corotation as a principal “driver" for the bimodal abundance radial distribution formation in the disk of our Galaxy . ...

XMM-Newton Science Analysis System . ... rgsrmfgen generates the response matrices. These are required by rgsfluxer for fluxing spectra, but their true value is seen in such sophisticated analysis packages as XSPEC, where a resolution of 3000 to 5000 incident energy bins (parameter rmfbins ) is recommended for good results. ... The default resolution is set high to avoid misleading the unwary, but lowering it to rmfbins =250 is highly recommended when fluxing is the only use intended. ...

... Head of the Department of Emission-line Stars and Galaxies of SAI MSU . ... Structure and kinematics of galaxies . ... Strasburg Database . Hubble Telescope Archive . ... CFHT Archive . ... Chinese evolutionary synthesis Yunnan . Korean evolutionary synthesis Yonsei . Evolutionary synthesis database BaSTI . ... Electronic Journal "New Astronomy" . Electronic Astrophysical Journal . Electronic Astronomical Journal . ... Questions and comments send to Olga Sil'chenko olga@sai.msu.su ...

... Asteroid . ... In case you didn't hear about it, which you probably didn't: On Jan. 7, an asteroid 1,000 feet across -- nearly three times the current diameter of Marlon Brando -- barely missed the Earth, which is most likely your planet of residence. ... What if this asteroid had hit the Earth? ... As it happens, the American Astronomical Society was holding a conference in Washington AT THE VERY SAME TIME as the asteroid nearly hit the Earth. ...

... Научная панорама ? astro-ph/07036663 Гигантский всплеск за два года до коллапса ядра массивной зве . ... astro-ph/07036663 Гигантский всплеск за два года до коллапса ядра массивной звезды (A giant outburst two years before the core-collapse of a massive star) . ... Близко от ядра М31. ... Световое давление направленное из ядра может просто сильно "надуть" звезду(повышение яркости из-за увеличеной площади излучения), но не "порвать" ее, тем самым оголив ядро.. ...