... N ear- I nfrared Camera ) с Laser Guide Star Adaptive Objects на обсерватории W. M ... Keck Observatory laser guide star adaptive optics discovery and characterization of ... ORBITS AND MASSES OF THE SATELLITES OF THE DWARF PLANET HAUMEA = 2003 EL61. ...
... с привлечением больших обзоров ( SDSS , 2 MASS и др.) исследовал строение и ... на горе Шатджатмаз , поддерживала программное обеспечение приборов DIMM / MASS ... CCD Observations of Four Stars Suspected in Variability from Digitized Moscow Plates ...
... Sun as a Star: Spectral Variability in the UV-VIS Range. Abstract . ... The analysis of experimental data obtained in studies of extrasolar low-mass ... number of detected planetans will grow as new exoplanets with masses of 1-5 Earth ...
... Surveys for stars and nebulae . · Extragalactic and cosmological surveys . ... STARS and NEBULAE . ... Tigran Magakian ( Armenia ) “Search for young stars and stellar objects” . ...
... использованы также инфракрасные данные в полосах JHK S , взятые из каталога 2 MASS ... вейвлет-анализа распределения звезд в каталоге 2 MASS , по данным JHK S -фотометрии ...
... Hierarchical star formation in M33: fundamental properties of the star-forming regions Monthly Notices of the Royal Astronomical Society, Volume 379, Issue 4, pp. ...
... M. S., Tuntsov A.V., Postnov K.A, Constraints on the massive graviton dark matter from pulsar timing and precision astrometry ... A.D. Chernin. Physics and Stars. 2004, 2002, Moscow, 'URSS'; 1983, Moscow, 'Nauka'. A.D. Chernin. Physics of Time. ...
... STARS: FROM ASTEROSEISMOLOGY TO SPACE WEATHER" to be held in 06-08 July 2015, Baku, Azerbaijan (Baku Solar Conference 2015) aims to highlight all aspects of modern solar physics research, including observation and theory that span from the interior of the ...
... A., Klochkov D., Wilms J. Variable neutron star free precession in Hercules X-1 from ... Elliptical motions of stars in close binary systems. http://arxiv.org/abs/1010.4452 ... Proceeding of the 41 conference on variable star research. ...
... P ~6yr, Delta(m) ~0.5m; quicker changes, P ~ 50d - 155d, Delta(m) ~ 0.3m - 1.0m. Together with the visual companion the star is surrounded by an enormous envelope (R ~2*10**5R$, expansion velocity 10 km/s, mass loss 3*10**(-8)M$/yr). nu Her [Fe/H] = -0.26 ...