... 314 ­ 321 Non­LTE Line Formation for Fe I and Fe I I in the Atmospheres of A­F Typ e Stars Mashonkina L. Institute of Astronomy, Moscow, Russia Abstract. ... Non­LTE leads to the Fe II lines strengthening, however, the effect is small, such that the abundance correction is at the level of -0.01 to -0.03 dex over the whole range of stellar parameters being considered. ... 2 What is Meant by the Non­LTE Approach? ... For the Fe I lines, we obtained the mean non­LTE abundance log FeI = 7.56 ± 0.09. ...

Change in Brightness Kepler 4b 0.0 % - 0.1 %0.12 - 0.2 % 0.14 0.16 0.18 0.02 0.04 0.06 0.08 Transit Light Curves Set 1 Transit Tracks p. 3 2 4 6 8 10 12 14 16 Time (in days ) 18 20 22 24 26 Change in Brightness HAT-P-7b 0.0 % -1.0% -2.0% 0.2 0.4 0.6 0.8 1.2 1.4 1.6 1.8 2.2 2.4 2.6 2 4 6 8 10 12 14 16 Time (in days ) 18 20 22 24 26 Change in Brightness HAT-P-11b 0.0 % -0.5% -1.0% ...

... 2010-01-20 . ... 2011 -01-28 . ... 2012-01-11 . ... 2013-01-05 . ...

TOPEX/Poseidon Jason-1 , , 14-17 2005 . ... 14-17 2005 . ... 110° 90°W. , , 14-17 2005 . ... 25° 25° 30° 30° 35° 35° 40° 40° 1.1993 1.1994 1.1995 1.1996 1.1997 1.1998 1.1999 1.2000 1.2001 1.2002 45° 1.2003 45° -0 .05 -0 .03 -0 .01 0 .01 0 .03 0 .05 0 .07 0 .09 / - 110°W. , , 14-17 2005 . 25° 25° 30° 30° 35° 35° 40° 40° 1.1993 1.1994 1.1995 1.1996 1.1997 1.1998 1.1999 1.2000 1.2001 1.2002 45° 1.2003 45° -0 .05 -0 .03 -0 .01 0 .01 0 .03 0 .05 0 .07 0 .09 / - 100°W. , , 14-17 2005 . ...

... 53, Moscow, 119991 Russia 2 MoscowPhysicotechnical Institute, Dolgoprudnyi, Moscow oblast, 141700 Russia Received June 15, 2004 ° Abstract--We present a catalog of 100 lines in the wavelength range 280­330 A detected by the RES-C spectroheliograph in solar active regions and flares during the SPIRIT experiment aboard the CORONAS-F orbital station. ... The line intensities recorded during the X3.4 (GOES) solar flare of December 28, 2001, are given. ... The Ca XVIII 302.19 A line is observed. ...

... DHOFAR 304, 305, 306 307: . Dhofar 304, 305, 306 307. ... Dhofar 302, 303, 305, 306 307. ... Dh-304 Dh-025 301, Dh-305, 306 307 Dh-081, 280, 302 303. ... Dh-305, 306 307 Dh-302 303, Dh-302 305 . ... MgO), FeNi (7.8 .% ... 1) (HMS) (FAN). ... FAN, HMS . ... Dh-306 FAN HMS (. ... Dh-305, 306 307 Dh-081, 280, 302 303. ... Dh-302, 303, 305 307 . ... Dh-305 307 Dh-303. Dh-305 307 (. ... Dh-305 (HMS) , Dh-307. ... 1) Dh-025, 301 304 ; 2) Dh-081 280 , , ; 3) Dh-302, 303, 305, 306 307 , Dh-302 305 . ...

Available online at www.sciencedirect.com Journal of the European Ceramic Society 29 (2009) 337­345 Single crystalline mullite fibres obtained by the internal crystallisation method: Microstructure and creep resistance S.T. Mileiko , A.V. Serebryakov, V.M. Kiiko, A.A. Kolchin, V.N. Kurlov, N.I. Novokhatskaya Solid State Physics Institute ... A special cross-sectional shapes of the fibres are shown in a series of the micrographs presented below to illustrate fibre microstructures (see Figs. ...

In the Table below the masses of some asteroids which were determined during the last years are listed. ... The listed values were determined from observations of many test bodies by the weighted least square fit for one perturbing mass and corrections to the orbit elements of all used test bodies. ... based on the observations of 98 asteroids (including 50278) with the values of standard error of mass determination less than 3.0 10 -11 M Sun . ... Mass . ... 3) Mass 121 : 0.74 x 10 -11 M Sun ; . ...

... The problems of complexity in coagulation: specification 1. ... Numerical experiments Task 1: Activation threshold Final clot density VS activation : model reduction Factor V is activated 7 6 7 6 No factor V activation Fibrin 4 3 2 1 0 0.00 0.02 0.04 0.06 0.08 0.10 0.12 Fibrin 5 5 4 3 2 1 0 0.00 0.02 0.04 0.06 0.08 0.10 0.12 Activation Activation y= Ae ( Bx 1 ) y = Ax Final clot density VS activation : the experiment Fibrin clot density (a.u.) 1.0 0.8 0.6 0.4 0.2 ...

... 15318 B9III 4.279 -0.056 -0.107 -0.023 -0.063 xi Cet "bs1544" 04 50 36.7 08 54 01 J2000.0 ! ... 34 239 sdG 11.225 0.488 -0.058 0.295 0.587 -0.030 -0.245 H "VMa2" 00 49 10 +05 23.4 J2000.0 ! 0046+051 LHS 7 DZ7 12.382 0.550 0.006 0.255 0.499 0.0812 -2.722 O "LTT1020" 01 54 48 -27 28.7 J2000.0 ! ... 2317-054 sdO 11.846 -0.304 -1.153 -0.133 -0.325 H,O !! ! ... 00 47 03.6487 -11 52 21.558 J2000.0(1999.5) 0.0 0.0 0.0 0.0 "BD-12" 00 52 15.3737 -10 39 48.039 J2000.0(1999.5) 0.0 0.0 0.0 0.0 "BD-11" ...

. Bright Supernovae - 2007 . This data comes from IAU Circulars and occasionally more data will be provided on IAU 's Astronomical Headlines page. An archive of the 2007 updates to this page is available. This is a list of the supernovae discovered in 2007. For supernovae which are still visible, please look at the main page for the latest data. Note that Extra galactic Novae have been moved to a special Extra galactic novae page . For more information, you can look at the following Supernova Catalogs: .

... Не менее интересны были соединения 17 июня 2 года до нашей эры и 13 сентября 1170 года, планета Венера проходит по диску Юпитера. ... В 30-градусном секторе встретятся сразу пять больших планет (Юпитер, Венера и Нептун, Марс, Сатурн) и Луна. ... МЕРКУРИЙ 0.16њ сев. планеты МАРС . ... ВЕНЕРА 0.55њ сев. планеты ЮПИТЕР . ... МЕРКУРИЙ 0.35њ южн. планеты ВЕНЕРА . ... МЕРКУРИЙ 0.13њ сев. планеты ЮПИТЕР Тройное соединение!! ... ВЕНЕРА 0.30њ сев. планеты МАРС . ... МАРС 0.36њ сев. планеты ЮПИТЕР . ...

Data online as files and in interactive forms in SPIDR The present catalogue contains information of avalability in WDC for STP,Moscow of data on neutron component of the cosimc ray intensity (corrected for pressure) in computer-readable form from 1957 --------------------------------------------------------------------- | ... USA | ... 0.00 | CANADA | ... FSU- Kaz.| ... FSU- Rus.| ... AUSTRALIA | ... ANTARCTICA | ... FRG | ... FSU- Ukr.| ... FSU- Uzb.| ... FSU- Geo.| ...

... Глава 2 . ... Ссылка из Главы 4 ). ... 0015+0501 . ... 0105+0501 . ... 19000 .008 . ... 3000 .010 . ... 450 .008 . ... 4000 .008 . ... 0444+0501 . ... 3000 .0502 . ... 3000 .011 . ... 0.64 . ... 3000 .014 . ... 12000 .008 . ... 1429+0501 . ... 1436+0501 . ... 3000 .034 . ... 500 .008 . ... 3000 .1613 . ... 1646+0501 . ... 1000 .008 . ... 3000 .0040 . ...

... Soc. 427, 790­805 (2012) doi:10.1111/j.1365-2966.2012.21990.x Ages and abundances in large-scale stellar discs of nearby S0 galaxies O. K. Sil'chenko,1,2 I. S. Proshina,1 A. P. Shulga1 and S. E. Koposov 1 2 3 1,3 Sternberg Astronomical Institute of the Lomonosov Moscow State University, Moscow, Russia Isaac Newton Institute of Chile, Moscow Branch, Moscow, Russia Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 OHA Accepted 2012 August 23. ... S0s fading from spirals. ...

... Сидерический . период . ... 0.01 . ... Ссылки . все данные взяты из работы 1, знак . отмечает данные из ссылки 2.) ... Astrometric and Geodetic Properties of Earth and the Solar System'' in Global Earth Physics, A Handbook of Physical Constants, AGU Reference Shelf 1 , American Geophysical Union, Tables 6,7,10. ...

... Exposure Time Calculator (ETC) . Survey processing . ... VISTA is a 4-m class wide field survey telescope for the southern hemisphere, equipped with a near infrared camera (1.65 degree diameter field of view at VISTA's nominal pixel size) containing 67 million pixels of mean size 0.34 arcsec and available broad band filters at Z,Y,J,H,K s and a narrow band filter at 1.18 micron. A wide field visible camera, if constructed, could also be used on VISTA. ... Tile . ... ESO VISTA Public Surveys . ...

... Number 5721 . ... 8 August 2006 . ... Data file: 5721-t3 . ... IBVS No. ... 2000.0 Max Min Type References h m s o ' m m 780217 V1675 Ori 05 34 23.8 -05 08 16 13.70 ( 0.08 ) Ic INB 072 USNO 780218 V1676 Ori 05 34 23.9 -05 15 40 11.19 ( 0.16 Ic) J INB 072 USNO 780219 V1677 Ori 05 34 24.3 -06 06 56 12.96 ( 0.10 ) Ic INB 072 USNO 780220 V1678 Ori 05 34 25.3 -04 54 39 13.24 ( 0.09 ) Ic INB 072 USNO 780221 V1679 Ori 05 34 26.1 -06 15 33 15.64 ( 0.14 ) Ic INB ... Sgr . ... Ori...

Общая Астрономическая Конференция > Практика > Астрономический наблюдательно-информационный портал > Хвостатые гостьи (все о кометах) > P/2014 K3 (SOHO) = P/2008 Y12 (SOHO) .. ... Просмотр полной версии : P/2014 K3 (SOHO) = P/2008 Y12 (SOHO) .. ... P/2014 K3 (SOHO) = P/2008 Y12 (SOHO), MPEC 2014-K37, CBET 3883 . ... Блеск кометы P/2014 K3 (SOHO) = P/2008 Y12 (SOHO) на момент открытия соответствовал н/д .. ... T 2008 Dec. ... K08CL C49 78.4+ 80.6+ Y K145H 249 13.1+ 3.6- Y K145H 249(15.8- 74.7-)Y . ...

... As these data span a large range in redshift, they are ideal for testing the validity of Type Ia supernova progenitor models with the distribution of expected \delay times," from progenitor star formation to SN Ia explosion, and the SN rates these models predict. Through a Bayesian maximum likelihood test, we determine which delay- time models best reproduce the redshift distribution of SNe Ia discovered in this survey. ... 1998) SD model. ... We tested two Gaussian delay time distribution models. ...