... Астронет | ... планета Астронет | ... S. Alba Villegas; R. Freire Ferrero . ... New insights on late-A and early-F star activity . ... Formation and stability of the galactic shock waves . ... Dispersion of electromagnetic waves in active moving plasma . ... N. G. Bochkarev; A. N. Burenkov; A. I. Shapovalova . ... The luminosity function of quasars (active galactic nuclei) in a merging model with the eddington limit taken into account . ... About the euro-asian astronomical society . ...

... ESO PR Photo 07a/01 . ... ESO PR Photo 07b/01 . ... Caption : PR Photo 07a/01 shows Comet Hale-Bopp , still active at a distance of nearly 2,000 million kilometres from the Sun. ... This is quite unusual for a comet and is clearly confirmed on the present photo ( PR Photo 07a/01 ) from the WFI camera on the MPG/ESO 2.2-m telescope at La Silla, obtained a few days ago. ... ESO-Chile . ... ESO PR Photos 07a-b/01 may be reproduced, if credit is given to the European Southern Observatory (ESO). ...

... 2004) Fire Radiative Power (FRP) · (Kaufman et al., ... MODIS active fire detections DNBR (MODIS (500m): 200,000 175,000 150,000 area burned (ha) 125,000 100,000 75,000 50,000 25,000 0 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 scar numbe r 200,000 175,000 MODIS dnbr ba (ha) 150,000 125,000 100,000 75,000 50,000 25,000 0 0 25,000 50,000 75,000 100,000 125,000 150,000 175,000 200,000 La ndsa t ba (ha ) y = 1. 0156x + 2069.1 R2 = 0.9925 Landsat ba (ha) MODIS af MODIS dnbr ba MODIS ba DNBR 1. ... FRP DNBR...

... 773Veron-Cetty Veron . Quasars (brighter than absolute magnitude -23) 85221 . ... Active galaxies (fainter than -23) 21737 . VII/248 Quasars and Active Galactic Nuclei (12th Ed.) (Veron+ 2006) ================================================================================ Quasars and Active Galactic Nuclei (12th Ed.) Veron-Cetty M.P., Veron P. =2006A .. ... 374, 92 (Catalogue ) (11) Veron-Cetty M.P., Veron P., 2003, Astron. ...

... Pre-university education . ... Samara region . SSAU History . SSAU roadmap . ... Samara State Aerospace University (SSAU) will take an active part in the work of space activities of the United Nations organization (UNO). ... The road map shape on inclusion of Samara University into implementation of the UN Program on Space Applications was outlined at the roundtable discussion with the University teachers and specialists and at the meeting with SSAU Rector Yevgeniy Shakhmatov. ...

... The active time at each angular bin is the sum over frames of the active time contributions from all CCD pixels, within the node-specific telemetry window, which overlap the surface of the bin. ... The active time, per frame, of a normal pixel is the full frame integration time multiplied by the node-specific fractional exposure; bad pixels contribute no active time. ... If an event is rejected for this reason only, then its pixels remain normal in the exposure map. ...

... VLBI Schedule . LBA Home Page . ... Observers Wiki . ... Main / . Parkes antenna control is via a command line program called atsnap. atsnap will run a simple schedule and can take commands to stow/unstow the antenna etc. ... Attenuation is done via the "loGUI" software. The VLBI backend consists of two "LBA DAS" which sample and filter the IF and the LBADR recorder which captures the sampled data, formats it in software and writes to local or remote disk (or streams for eVLBI). ...

HST MOSES July 30, 2003 CHAMP/MOSES SM4 SMOV Requirements PCS TCS ASCS DMS 1 HST MOSES PCS L.10.4.8 J Wirzburger July 30, 2003 L.10.4.8 Pointing Control Subsystem Verification Requirements: PCS ­ L.10.4.8.1 Following release, the HST Pointing Control System will be returned to normal operations for SMOV with four gyros in the active control loop, (no shadow mode). A fine attitude reference will be uplinked to the spacecraft and the spacecraft will be maneuvered to point to the BEA attitude. ...

... VISA APPLICATION . ... The following documents should be usually submited to the Russian Embassy or Consulate to obtain a Business Visa to enter Russia: . Tourist invitation or business invitation issued by an organization authorized to invite visitors to Russia. ... An official business invitation must be only issued by the Russian Foreign Ministry or its regional representatives or by an appropriate Russian Federation Migration Service branch. ... The deadline is November 5, 2013 . ...

... Monitor ID Bit 3, TTL . ... Composite Sync (Active Low), TTL . ... Horizontal Drive (Active High), TTL . ... Vertical Drive (Active High), TTL . ... Digital Ground . ... Sync Ground . ... Composite Sync . ... Horizontal Sync . ... Vertical Sync . ... DDC Ground . ... Chassis Ground . ... SGI Octane Workstation Owner's Guide . ...

... Артикул 3466602Из . ... Основной материал: Бижутерный сплав . Вид товара: Бижутерия . Материал: Бижутерный сплав . ... Цвет: хаки . ... Материал верха: искусственная кожа, текстиль . ... Рюкзак DKNY Active. ... Материал: искусственная кожа, текстиль. ... Линейка: Active . Прием сигнала HDTV: н/д, Цвет: белый, Бренд: HAMA . ... Цвет: Красный . ... Цвет: рисунок флаг британский . ... USB 2.0 Apacer AH324 32Гб, Красный, пластик, USB 2.0 32Гб, Красный, пластик, USB 2.0.. USB флешки . ...

... astro-ph . ... We present the goals and preliminary results of an unbiased, near-infrared, narrow-band imaging survey of the First Galactic Quadrant (10deg<l<65deg ; -1.3deg<b<+1.3deg). ... We publish 16 Doppler imaging temperature maps for the years 1994-2002 of the active RS CVn star II Peg. ... Through Doppler imaging we want to study the spot evolution of the star and in particular compare this with previous results showing a cyclic spot behaviour and persistent active longitudes. ...

... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. 2001 October 16 . A Newly Active Volcano on Jupiter's Io . ... Explanation: Would a volcano plume discovered in January above Jupiter's Moon Io still be active months later? ... Careful inspection of the two images will show a newly prominent dark volcano surrounded by a light-colored ring visible only in the smaller, more recent image . ...

Proposal Identi cation No.: A1167 Date Received: 1998-Jun- 1 19:31:20 Technical Page Proposal Type: Regular General Category: Astronomy Sub-Category: Spectroscopy Observation Category: Extragalactic Total Time Requested: 39 Hours Proposal Title: EVOLUTIONARY TRACKS OF ACTIVE SPIRAL GALAXIES ABSTRACT: Recent work has shown that the disks of Seyfert host galaxies follow trends of HI mass fraction, surface brightness, and M/L ratio similar to, but o set from, those in normal spirals. ...

... The chromospheric contribu­ tion to Li I lines in active dwarfs E.R. Houdebine and J.G. Doyle In magnetically active stars, non­thermal heating and magnetic fields result in inhomogeneous outer atmospheres (plages) and photospheres (dark and bright spots. ... Solving the NLTE­radiation transfer problem for a grid of model atmospheres that mimic the effect of magnetic activity (from basal to saturated chromo­ spheres), we show that the Lithium lines are in fact activity sensitive. ...

Next: Feature enhancement: local Up: No Title Previous: Feature enhancement: filtering . ... As a result, a common magnitude scale (contour lines on the maps above, or color scale on Fig.1) will poorly display the short-duration events in a signal. Normalizing each line of the map (fixed duration) so it has unit variance (in effect dividing the energy map by the mean energy spectrum) at each duration restores more details of small-scale activity (Fig. ...

... The effect of the normal star on the compact magnetized component is largely determined by the rate and velocity of stellar wind at infinity . ... For Be-stars (i.e. those stars at the stage ``I'' whose mass increased during the first mass exchange), the wind velocity at infinity is taken to be equal to the Keplerian velocity   at the stellar surface . Thus, the lower stellar wind velocity leads to an effective increase of the captured mass rate by a secondary companion to such Be-stars. ...

. Assumed Source Spectra (2-10 keV): . Normal AGN: a x = 0.5, N H = 3 10 20 cm -2 . Absorbed AGN: a x = 0.5, N H = 3 10 23 cm -2 . An explanation of and further information on these predictions can be found here . Sky Area vs. flux limit (0.5 - 3.5 keV) . Sky Area vs. flux limit (2 - 10 keV) . Home | Science Goals | Survey Strategy | Publications | Images & Data | Education/Outreach | Internal Page (password access only) . Date Last Modified: 22 April 2002 . Contact: Webmaster .

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... 1994: . As a result of comparing the spectra of active solar regions from the observations with high spatial resolution in the microwave range at the RATAN-600 (the S-component) with a flare component observed at meter wavelengths on the VLA (USA) we revealed the presence of a strong and prolonged noise storm exactly where a weak decaying active region (with the presence of powerful active regions in the disk) is located. ... Archive . ...