... part 1 | ... Part 3 . The new circuit of global tectonics of the planets and their satellites . ... The "too hot" substance (magma) is formed of combination of different sort of atoms of chemical elements, spontaneously arising in the entrails of the pre-Earth cosmogenic vortex (and equal in entrails of other celestial object of spherical form). ... The water dropped out from the last it gradually was condensed and formed the widths of uniform Global ocean. ...

On properties of metallicity function of F-stars in the galactic disk . Yu.Shevelev & V.Marsakov . ... MF of different age disk stars . ... Age-metallicity relation . ... Based on the complete sample from ( Marsakov & Shevelev, 1995a ) we determined in ( Shevelev & Marsakov, 1995 ) the vertical metallicity gradients of disk population stars in several narrow age ranges from the observed metallicity values and the calculated maximum distances of their orbits from the galactic plane. ...

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St. Petersburg, Russia, June 27-30, 2011 . ... Program committee . ... The International Academy of Astronautics created a SETI committee in the seventies now established in Permanent Study Group. ... The Committee reserves the right to reject paper or to change form of its presentation. ... The registration fee includes conference materials, coffee breaks, welcome party, transportation and dinner while visit to "Svetloe" observatory, book of abstracts, conference program, volume of Proceedings. ...

including instructions for authors and subscription information: http://www.informaworld.com/smpp/title~content=t713453505 Space- time distributions of the coronal green-line brightness and solar magnetic fields O. G. Badalyan a; V. N. Obridko a; J. SЩkora b a Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, Troitsk, Russia b Astronomical ... Characteristic CGLB synoptic charts for cycle 21. ... SPACE­TIME DISTRIBUTIONS OF CGLB AND SOLAR MAGNETIC FIELDS Table 2. ...

... FTP access the basic models is here . ... Below, we put short descriptions of the used SED models for the photometric redshifts providing by the current server . ... The uniqueness of this model consists in expanding to the near IR (NIR) of Rocca-Volmerange and Guiderdoni's (1988) atlas of synthetic spectra with a revised stellar library, which includes parameters of cool stars. ... Homepage of the GISSEL model). ... Another model used earlier is the model of synthetic spectra of Poggianti (1997). ...

. Английская версия . Последнее обновление в мае 2008 г. Проект РадиоАстрон .

... Exposure Time Calculator (ETC) . ... ESO - Public Surveys . ... the recommended values to use for DIT, . ... Detector on-chip integration (DIT): seconds. to your chosen value - a separate page gives recommended values to use for DIT - for modes 1 and 2 below you may wish to start with the maximum recommended values as these will minimize the effect of read noise (a total object exposure of Y secs with DIT=X secs will produce Y/X lots of read noise) and give you a lower limit on the time needed. ...

... VaST is a software tool for finding variable objects on a series of astronomical images. ... VaST performs object detection and aperture photometry using SExtractor on each image, cross-matches lists of detected stars, performs magnitude calibration with respect to the first (reference) image and constructs a lightcurve for each object. ... VaST FITS image viewer ./pgfv . ... Part I" PZP, vol. ... K. V. Sokolovsky, S. A. Korotkiy; "New Variable Stars Discovered by the NMW Survey" PZP, vol. ...