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 picture shows sketches of the optical and ultraviolet (top, left) and X-ray (top, right) spectra of a typical quasar or AGN (Active Galactic Nucleus). These spectra are full of sharp features due to the interaction of atoms with light ('atomic features'). They can be high (= bright) points, called 'emission lines' or low (= dark) points, called 'absorption lines' . ... Broad Emission Lines ("BELs") [seen in 100% of AGN], . ... Broad Absorption Lines ("BALs") [see in only 10% of AGN], . ...

... Кресла . ... Размер: XS . ... Цвет: белый . ... Размер шлица: PZ2 ; . ... Цвет: Фиолетовый . ... Глубина: 90 . ... Цвет: черный . ... Цвет: серый . ... Размер INT: 54 . ... Глубина пропила: 90, . ... Макс. глубина пропила под углом 90њ: 90, . ... Размер площадки: 800x550, . ...

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... The algorithm and appropriate program for decametric radiosignal propagation conditions prediction for paths from 500 to 9000 km have been developed at ISTP SB on the basis of normal wave method (AltyntsevaB.I,Iliyin N.V., Kurkin V.I. and others //Decameters channel simulation on the base of normal wave method . ... Solar activity indices are chosen automatically from the prediction date from the database . ...

... ones: H2, C2, C3 Diffuse interstellar bands (known since 1922) Unidentified; Proposed carriers: carbon chains, PAHs, fulleranes Radial velocity of CH+ can be different than those of other species 1.6 RbI 7800A*3 CN 3875A Relative intensity 1.4 CH 3886A CH 4300A/2 1.2 FeI 3720A CH 3957A 1.0 + CH 4232A HD152932 ESO UVES -60 -30 0 30 60 + Radial velocity Diffuse bands (strong and weak) may be of different origin(s) 5780 5772 5775 5797 HD147165 5795 1.02 Relative ... CH 0.96 DIB? ...

... Field of research: Extragalactic astronomy. ... NASA Astrophysics Data System (ADS) Abstract Service . ... CADC Home Page . ... CCD Images of Galaxies . ... RUSSIAN LINKS . ... UA Astronomy Personal Home Page - Bill Keel . ... The Shape of the Rotation Curves of Edge-on Galaxies, by A.V.Zasov and A.V.Khoperskov, 2003. ... A Thickness of Stellar Discs, by A.V.Zasov, and D.V.Bizyaev, 2003 . Minimum Velocity Dispersion in Stable Stellar Disks, by A.V.Khoperskov, A.V.Zasov, and N.V.Tyurina, 2003 . ...

. [ Go back to Comet WWW site ] . Andrew A. Martis . martis @ sai.msu.ru .

... R-band images obtained at 0.8 arcsec seeing conditions have allowed us to separate foreground star from point-like extragalactic source and estimate their brightness separately. ... To study the nature and properties of the source, we observed it under high spatial resolution. ... CONCLUSION RTT150 optical observations with sub-arcsecond seeing and low resolution spectra confirm the hypothesis of superposition of a radio source onto a `normal' F/G galactic star proposed by [1]. ...

Magnetic Stars, 2011, pp. ... Key words: stars: pre­main­sequence ­ stars: atmospheres ­ stars: individual: HD 101412 ­ stars: magnetic fields ­ stars: rotation ­ stars: variables: general 1 Intro duction In our previous studies we reported detections at a level higher than 3 for three out of seven Herbig Ae stars observed with the low­resolution spectropolarimeter FORS1 at the VLT (Hubrig et al., ... This is the first time the presence of element spots is detected on the surface of a Herbig Ae star. ...

The most up-to-date information related to atmos 3.0 are collected here due to constantly increasing interest to MASS/DIMM processing software... atmos 3.0 is still beta , so the latest version is 2.97.5 (there is also 2.98.x branch which absorbs new features) . ... M' line: . ... free seeing and its relative error . ... dimm seeing and its relative error (if dimm data are present, zeros otherwise) . ... dimm turbulence power and its relative error (if dimm data are present, zeros otherwise) . ...

Stellarium 0.12.3 . ... Renderer . FileљStructure . ... core . ... StelVertexAttribute.hpp . ... 53 љ inline int attributeDimensions( const AttributeType type) . ... 122 љ qDebug() << "Unknown vertex attribute type: \"" << typeStr . ... 179 љ // Ensure that every kind of vertex attribute is present at most once. 180 љ foreach ( const StelVertexAttribute & attribute, attributes) . ... 186 љ "Vertex type has more than one vertex position attribute" ); . ... 239 љ #define VERTEX_ATTRIBUTES(...)\ . ...

. Russian . English .

... For a semple of red giants comprising about 2000 stars, the distributions of metallicity [Fe/H] are given. ... The center of the distributions of giants in both galactic poles is found to demonstate a statisticaly significant gap similar to the one found earlier for the late main-sequence stars. The implications of the metallicity distribution properties for the problems of the chemical evolution of the galactic disk are discussed. ...

Small Galaxy Groups ASP Conference Series, Vol. ... It is generally accepted that they are related to the nuclear rings formed in barred galaxies at the inner Linblad resonance (ILR), although according to Buta and Crocker (1993), in some cases they were found in non-barred spirals, so in general a presence of large-scale non-axisymmetric gravitational potential is not a rigid condition for the nuclear bar to be formed. Typical length of nuclear bars is 1 - 2 kpc for H 0 = 75km=s=Mpc. ...

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VIEW OUT OF THE WINDOW FROM ALBUQUERQUE, NEW MEXICO, USA . The winter started early here with severe snow storms in November and December. ... But this winter we had so many storms, food had to be air-lifted by the Air Force, to feed farm animals in the countryside. The weather began to get much better in January. Now it is cool and sunny. ... New Mexico is usually very dry, . ... This altitude, coupled with the dry sunny climate, results in very cold nights and cool days in the winter. ...

. Prague, August 16, 2006 . Present classification : Suggested: . SN, SNI, SNII SN (to avoid introducing the current complex classification) AM AM (including XM from X-ray variables), DQ (intermediate polars) . UG, UGSS, UGZ UG, UGSS, UGZ UGSU UGSU, UGWZ (WZ Sge type, extremely long supercycles, large amplitudes), UG_ER (ER Uma type, short supercycles and normal cycles, small amplitudes; ideas of a better abbreviation are welcome) . CATACLYSMIC VARIABLES . AND OTHER STARS WITH OUTBURSTS (CONTINUED)

... 3rd ISCC) Kunming, China, Oct. ... THIRD INTERNATIONAL SYMPOSIUM OF CHRONOBIOLOGY AND CHRONOMEDICINE Kunming , China , October 7-12, 1998 REGISTRATION FORM This form should be typewritten Participant Title (tick): Prof. _ Dr. _ Mr. _ Mrs. _ Miss _ Ms. _ Surname: _______________ ... ____________________ Given name(s): ______________________ Country: _____________________ Nationality: ________________________ Registration fees: Participant Companion N of companions Amount U.S . $300 ...