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... Mass modeling shows that the contribution of the stellar component to the rotation cur ves may be scaled to explain most of the inner parts of the rotation cur ves, albeit with high stellar mass-to-light ratios. ... L107 L108 HIGH-RESOLUTION ROTATION CURVES Vol. ... The relative contribution of the stellar disk to the rotation cur ve may change continuously from LSB to HSB, or perhaps LSB and HSB galaxies constitute discrete galaxy families, as has been suggested by Tully & Verheijen (1997). ...

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University Satellites and . Space Science Education . ... Abstract Submission List of submitted abstracts . ... The abstract you have submited . The 19th century observation of light phenomena versus space-time continuum. ... The author show endeavours for adjustments of optical phenomena and electrodynamics processes with the 19th century concept of ether. ... Skobeltsyn Institute of Nuclear Physics, Moscow State University, 2005-2006 . ...

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... V.V.Shevchenko, Sternberg State Astronomical Institute, Moscow University, Universitetsky 13, Moscow 119899, Russia, shev@sai.msu.ru . ... 1.Sternberg State Astronomical Institute, 119899, Moscow, Russia. shev@sai.msu.ru . ... V.V.Shevchenko, Sternberg State Astronomical Institute, Moscow University, Moscow 119992, Russia, shev@sai.msu.ru . ... 119992 Moscow, Russia; . ... 2Sternberg Astronomical Institute, Moscow University, Moscow, 119992, Russia, . ... Moscow, 119992, Russia shev@sai.msu.ru . ...

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Date: Thu, 12 Apr 2007 18:15:45 +0200 (MEST) From: Alessandro Marconi <marconi@arcetri.astro.it> To: boch@sai.msu.ru Subject: Summer school on AGNs and VLTI Dear Colleague, here is the first announcement and call for applications for a VLTI summer school on "Active Galactic Nuclei at the highest angular resolution: theory and   observations". ... It is supported by 15 EU member states, including new member states, and thus integrates the entire European optical interferometry community. ...

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... Envisat contributes greatly to scientific research with its ability to monitor environmental and climatic changes on a global scale. ... Envisat has captured many environmental is- "Satellite images can determine whether fires in certain locations need monitoring" Figure 2 shows Portugal and Northern Spain; the white wisps moving across the Atlantic are smoke from fires that devastated this loca- Image Credit: ESA 2 Astronotes November 2007 tion in August 2006. ... Image Credit: ESA Figure 2. ...

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Some comments on the direction of p olarization in the coronal green line O.G. Badalyan Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, 142092 Troitsk, Moscow Region, Russia Received: December 31, 2001 Abstract. ... The direction of polarization in the green line turns out to be tangential, i.e., the same as in the white-light corona, virtually everywhere except in the bright equatorial regions. ... Direction of p olarization in the green line 3.1. ...

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sw@newmail.ru THE PROBE LAYER METHOD IN THE CALCULATIONS OF CONTRIBUTION AND RESPONSE FUNCTIONS S.G.Mozharovsky Ussuriysk Astrophysical Observatory of FEB RAS, Ussuriysk, Russia sw@newmail.ru The method of probe layer for the calculation of response and contribution functions is discussed. ... This allows us to turn from the response functions to the contribution functions calculated with help of the probe layer (CFPL). ... V- VMAX . ... Solar Phys., v.136, p.239-250. ... Solar Phys., v.35, p.11-29. ...

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ПУБЛИКАЦИИ - 1994 год . G.Ya.Smolkov , V.P.Nefedyev, A.M.Uralov , N.N.Kardapolova. Step-wise emergence and development of microwave emission of active regions-a fundamental property of active solar corona. Solar coronal structures, Proc of 144th IAU Coll, Veda, Publhouse of SAS, - 1994. ... The observations of solar microwave bursts at the Siberian solar radio telescope with 50-millisecond resolution. ... Nato Rubl/Nauka, - 1994. ... Electron beam propagation in the solar corona. ... 1994. ...

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Elsevier Ed itorial System(tm) for JASR 2006 Manuscript Draft Manuscript Number: Title: Determination of K, Ar, Cl, S, Si and Al flare abundances from RESIK soft X-ray spectra Article Type: Contributed Paper Section/Category: E2.4 - Solar Magnetic Field and Activities Keywords: solar physics; X-ray flares ; spectroscopy; abundances Corresponding Author: Dr. J. Sylwester , Corresponding Author's Institution: Space Research Center First Author: J ... All flares were observed early Fig. ...

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... Fig. 3) suitable for estimating the brightness temperature. ... Ir ­ brightness distribution function; T b ­ brightness temperature estimated from Ir ; Vq ­ visibility function; dq ­ pattern size, estimated from the visibility ratio Vq /V0 ; T b,q ­ brightness temperature corresponding to dq ; T b,min ­ minimum brightness temperature, obtained with V0 = eVq for the Gaussian component and V0 = 2 Vq for the disk and the shell; T b,lim ­ limiting brightness temperature, obtained with V0 = Vq + q . ...

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OSLO LT V5.4 Optical Software For Layout And Optimization . Articles | ... Has anyone out there tried to raytrace a telescope design? ... OSLO LT keeps track of the optical path length each ray travels, so it knows the phase relationship of the light as it travels through the telescope. ... Through the use of OSLO LT, I've been able to refine the optical design of the telescope I'm working on. ... www.astronomy.net . About Astronomy Net | ... dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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... for Cosmic Ray Observation is situated in Irkutsk (Russia). ... Real-time (preliminary) cosmic ray data in Irkutsk . ... Online Cosmic Ray and Atmospheric Pressure Data Base . ... Real-time data Uncorrected for pressure (Resolution 1 hour - 1 year) -- since 05.2001 . Real-time data Corrected for pressure (Resolution 1 min - 1 year) --- since 09.2001 . Resolution 1 hour - 1 year) --- since 06.2001 . Final data Corrected for pressure (Resolution 1 hour - 1 year) --- From 01.1975 To 07.2004 . ...

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... By undertaking a spectral and photometric investi­ gation of the central part of the bright elliptical galaxy NGC 759, we have found an optical counterpart for the circumnuclear molecular gas ring with the radius of # 3 ## (# 1 kpc) which was earlier reported by Wiklind et al. ... 2 Fig. ... More likely, this ring may be a consequence of a tidal encounter between the elliptical galaxy NGC 759 and a large spiral galaxy which was accompanied by a substantial gas accretion. ...

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