... 2008 October 9 . Massive Stars in NGC 6357 . ... Explanation: Massive stars lie within NGC 6357 , an expansive emission nebula complex some 8,000 light-years away in the tail of the constellation Scorpius . In fact, positioned just below center in this close-up view of NGC 6357, star cluster Pismis 24 includes some of the most massive stars known in the galaxy , stars with over 100 times the mass of the Sun. ... About APOD | ... NASA Official: Phillip Newman Specific rights apply . ...

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... Credit Copyright: NASA 's Goddard Space Flight Center , CI Lab Explanation: What happens when a star gets too close to a black hole? ... Although angularly unresolved, variations in high energy light indicate that some of the star became shredded and reformed into a disk swirling around the dark abyss. ... Publications with keywords: black hole - accretion disk . Publications with words: black hole - accretion disk . ... Two Black Holes Merge . When Black Holes Collide . ...

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... October 18, 1999 . NGC 3603: An Active Star Cluster . ... Explanation: NGC 3603 is home to a massive star cluster, thick dust pillars, and a star about to explode . The central open cluster contains about 2000 bright stars, each of which is much brighter and more massive than our Sun . ... These stars are less massive than our Sun, demonstrating that great numbers of low-mass stars also form in active starburst regions . ... About APOD > . ...

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Supernova 2009js in NGC 918 . This page is devoted to information on Supernova 2009js in NGC 918 . Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main page . Information on the original web pages for many of these images can be found on the updates and links web pages. Discovered independently by Lick Observatory Supernova Search (USA) and Koichi Itagaki (Japan). ... 2009/10/11.44 . 17.2 . ... Joseph Brimacombe . ...

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... An hour later, the satellite has proceeded to higher altitudes and the auroral proton precipitation pattern can be seen, using the SI-12 proton imager. ... The IMF dependence of the proton cusp signature has been described at length recently in several papers by Frey et al. [2002, 2003]. movie of this event This is just the first indication of activity and this storm is a continuing event, now with (a possibly unprecedented) 2 successive dips of DST below -300 nT. ... Proton aurora in the cusp . ...

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... 28 March 2014: release of Volume 13: new photos and drawings , new published papers . 12 September 2012: release of Volume 12: new photos and drawings , new published paper , new list of invertebrate animals . ... 28 September 2010: release of Volume 10: updated bibliography , new photos and two new articles appeared: on Drosera and on Nymphaea . ... 29 September 2006: release of Volume 6: new photos , updated map , updated bibliography and updated list of the invertebrates . ...

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Effective Algorithm of Charge State Determination in Electrospray Ionization Fourier Transform Ion Cyclotron Resonance Mass Spectra of Humic Substances Erast V. Kunenkov1, Andras Gaspar2, Alexey S. Kononikhin3, Philippe Schmitt-Kopplin2, Irina V. Perminova1 ... ESI FTICR mass spectrum of HS contains about ten thousands of peaks in mass range 250ґ1200 Da (the most intensive peaks are usually located near 400 Da) with tenths of peaks, appeared at each nominal mass with high regularity. ...

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. To see a Russian version of this page click here . (Senior Researcher. Graduated from Moscow State University (MSU) in 1982, Ph.D. 1986, MSU) . A member of EAS and IAU. Fields of interest: hot massive stars, close binary systems: optical photometric and spectral observations, X-ray observations; ill-posed problems, X-ray astrophysics. My publications (ADS link) . Linux on CLEVO 8750 (old stuff) . Phones/addresses of my university mates graduated in 1982. E-mail: igor@sai.msu.ru .

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... Academic Departments . ... Partners . ... All partners . ... 21.10.2014 On October 17-18, 2014 the Faculty of Journalism of Lomonosov Moscow State University hosted The 6th International Media Readings in Moscow Mass Media and Communication-2014 . The overarching theme of the conference was ?Creative Industries in the Reindustrializing World: Media Practices of the West and the East? ... The speech of Terry Flew was organized as a pre-conference of Moscow Readings event. ...

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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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THE ARGUMENT AGAINST LONG EXTRAGALACTIC DISTANCE SCALE Gaseous discs of S0 -- Sd galaxies appears to be gravitationally stable or close to stability. Dependence of the gravitational stability parameter of gaseous disc $M_g/M_c$ upon the color index $(B-V)^0_T$ which reflects a relative number of young stars, is found. Here $M_g$ is total mass of gas in a galaxy, $M_c$ - mass of gas which corresponds to marginal stability of gaseous disc at distances from center. ...

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... So one can describe neutrino by a Majorana field which has the same number of degrees of freedom as a left Dirac one. ... neutrino . ... In terms of Dirac field a neutrino appears in the Standard Model Lagrangian in the following way ( .19 ) 1 : . ... To rewrite it in terms of a Majorana fermion let us perform the substitution . ... G(m3)*(1-G5) . ... Let us emphasize that there are two identical neutrino fields in that term of the Lagrangian which describes the interaction of neutrinos with a ...

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Comparative mineralogy of carbonatite complexes belonging to different formations . ... I. Within well known formation of ultrabasic -alkaline rocks within carbonatites (UAC), the main rare metal ore components are Nb, Zr, REE Ce , rarely Sr, Ba, U, Ta, Th, as well as phosphorus in apatite, in zones of hypergenesis ? minerals of crandallite group and others; fluorite, Fe in magnetite, rarely hematite and its hydroxides, sulfides of non-ferrous metals ? Cu, Zn and others. ...

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