... We revised topographical data obtained for the region to construct a generalized structure of the SPA basin as ringed formation. ... Because of our previous analysis of the ring structure [5, 6] we assumed the projection center o o coordinates as 180 W and 40 S. The hypsografic map shown in Fig. 1 demonstrates a hemisphere of the Moon which contains the SPA basin structure and its environs. ... Then we find the o o basin outermost ring center at roughly 180 and 40 S. Inner structure of the SPA basin...

... Reports on progress and error are always recorded in the log file of the program. ... UT date of the measurement finish in YYYY-MM-DD format UT time of the measurement finish in hh:mm:ss format Average flux in A aperture Average flux in B aperture Average flux in C aperture Average flux in D aperture Normalized variance of flux in A aperture Normalized variance of flux in B aperture Normalized variance of flux in C aperture Normalized variance of flux in D ...

... 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. ...

. Comment on J0431+2037 . A Gigahertz Peaked Spectrum (GPS) galaxy with complex radio structure on the scale of 10 to 100 mas (combined EVN+MERLIN data at 1.6 GHz, Dallacasa et al. 1995). Our image is consistent with the center-southern features of Dallacasa et al. (1995). The northern feature, ~180 mas N-NW from the field center, outside the boundary of the displayed image, can barely be seen in our data. VLBApls home page . Last modified: 16 Oct 2000

. home . product . gallery . contact . Telescope rc360 . Telescope rc400 . Telescope rc500 .

Configuration Files | ... Options | ... This version of Apache includes changes allowing it to run on IBM's EBCDIC-based TPF (Transaction Processing Facility) operating system. ... It is passed to Apache through the ZINET XPARM field since ZINET is the only way to start the server on TPF. A third group of options apply to both the informational displays (ZFILE) and running the server (ZINET XPARM): -d, -D and -f. The rest of Apache's options are either not applicable or are not supported on TPF. ...

August, 2012, Odessa, Ukraine EVENTS: Monday, 20.08.2012 Arrival 09.00 ­ 22.00 Registration of participants 20.00 ­ 22.00 Evening session : Astronomical Society news (conference hall of ONU recreation center « Chernomorka ») Tuesday, 21.08.2012 06.03 09.00 09.30 10.45 12.45 13.00 14.30 16.00 16.30 18.00 19.00 19.57 21.00 06.04 09.30 11.00 11.30 13.00 14.30 16.00 16.30 18.30 20.00 19.56 ­ ­ ­ ­ ­ ­ ­ ­ ­ ­ 13.00 10.45 12.45 ... 10 Section 3. ... 14.30 ­ 15.30 Section sessions ­ .. ...

... SB, Porb = 55.9212d. V0745 Cas| ... Component B of the double system observed brighter than in the Hipparcos Input Catalogue. ... The variability may be due to the fainter component. ... Type ELL: is also possible. pi Cas| ... Variability type and spectral type (F2/F3Ib/II) do not agree. ... Variability type and spectral type (F3/F5II) do not agree. ... Variability may be due to component B. VZ Pic| ... Variability may be due to component B. V1377 Ori| ... SB, Porb = 9.073d. V0421 Cep|105091| ...

АНОНС КОНФЕРЕНЦИЙ PRELIMINARY ANNOUNCEMENT Current Problems in Astrophysics International Scientific Meeting in memory of three distinguished Astrophysicists: 80th birthday Professor I.S.Sklovskii and to the 75th birthday of Professors S.A.Kaplan and S.B.Pikelner September 23-27, 1996 , Moscow , Russia Sternberg Astronomical Institute of Moscow Lomonosov University Astro-Space Center of P.N.Lebedev Physical Institute Euro-Asian ... 13, 119899, Moscow. ...

. Institute Structure . • Administration . • Research Divisions: . Superhigh energy particles . Space plasma physics . Aeronomy . • Center of information technology . • Stations: . Yakutsk Extensive Air Shower (EAS) Array . Polar Geocosmophysical Observatory (PGO) . Complex Geophysical Station (CGS) . Optical Station . Yakutsk Cosmic Ray Spectrograph . Magnetic Observatory . Ionospheric Station . Station for Receiving of Satellite Information .

Астрономия и Космос Небесные тела Черные дыры и пульсары . А строномы получили наблюдательные подтверждения того, что некоторые черные дыры вращаются вокруг своей оси , подобно водоворотам. ... Следовательно, черные дыры , как и нейтронные звезды, могут вращаться вокруг своей оси . ... Комментарии к Черные дыры вращаются вокруг своей оси . Ссылки по теме Черные дыры вращаются вокруг своей оси: . Черные дыры вращаются вокруг своей оси . Черные дыры и пульсары . Имитация черных дыр . ...

Statistics of sunspot activity . The sunspot indices . ... NGDC's observations . The solar regions . ... Average annual indices . ... December . ... December, 2013 . Visual indices of solar activity by National Geophysical Data Center . ... Average . ...

... Астрософт (Модератор: tlgleonid ) > . Celestia или как там ее . ... Right drag: orbit the selected object . ... Ctrl + Left drag: adjust distance to selection . Shift + Left drag: change field of view (e.g. => telescopic view) . Wheel (middle button) click: toggle field of view between 45 degrees . ... Chase selected object (orientation is based on selection's velocity) . T : Track selected object (keep selected object centered in view) . ... Ctrl+P : Mark selected object . ...

... 24 } Line { SrcBlock sin SrcPort 1 DstBlock func1 DstPort 1 } Line { SrcBlock Fcn SrcPort 1 Points [0, -55] DstBlock func DstPort 1 } Line { SrcBlock (G*M) ^1/2 SrcPort 1 Points [25, 0] DstBlock func DstPort 3 } Line { SrcBlock func SrcPort 1 Points [40, 0] Branch { ...

Title: A Dark-Matter Spike at the Galactic Center? Authors: Piero Ullio , HongSheng Zhao , Marc Kamionkowski . ... Title: The Galaxy Environment of Quasars in the Clowes-Campusano Large Quasar Group at z~1.3 . ... Title: The Galaxy Environment of a Quasar at z=1.226: A Possible Cluster Merger . ... 16 matches for the search pattern galaxy environment . The URL for this page is: http://xxx.itep.ru/find/astro-ph/1/galaxy+environment/0/1/0/past,all/0/0 www-admin@xxx.lanl.gov ...

RUSSIAN . The Centre for Astronomical Data (CAD) of the Institute of Astronomy (INASAN) of the Russian Academy of Sciences was established in 1980 as a branch regional center of the Centre de Donnes Stellaire (CDS) with the purpose of astronomical data dissemination among Soviet and Eastern Europe astronomers and for providing the CDS with Soviet machine readable astronomical catalogues. The CAD archive is based on astronomical catalogues received from Strasbourg since 1980. ...

... Luna-9 lander . ... Luna-16,20,24 return capsules . ... Luna-16 drill . Luna-16 drill cutaway . Luna-16 drill base . ... Luna-17 . Luna-17/21 closeup . Luna-17/21 ramp . Luna-17/21 top view . Luna-17/21 bottom view . ... LK landing leg shock absorber . ... LK engine . Krechet detail . Krechet lunar suit . ... Venera-8 lander . ... VEGA TV platform . Venera-2..-7 engine . ... VEGA lander . ... Vega baloon probe . ... Mars/Venera engine . ... Mars-3 lander . ...

... Center-Limb Variations ! ... Оцифрованы данные из книги Гуртовенко и др. 1975г ! ... Сформулированы ближайшие направления развития SunWorld ! ... В проект добавлен раздел GEDA - Общие данные ! ... в расчет все линии диапазона ! ... Начата обработка списков линий Kurucz на предмет ! включения в БД SunWorld лишь тех линий, которые ! ... с) Можаровский С.Г. // mailto:sw@newmail.ru // Home page Solar page ...

... part 2 | ... Part 1 . The new concept of formation and development of the Solar system. ... Thus, the initial pulse of the rotation of a protosolar cloud of the solar system was determined as a result of the diversion of a part of the moment of the rotational pulse of the Galaxy. ... Besides this new approach to the pre-solar system as a system of the destroyed vortex structure, we can understand now a number of other peculiarities of the Solar system's structure. ...

... 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 . ...