Peremennye Zvezdy ( Variable Stars ) 33 , No. ... I present the discovery of an eclipsing component in light variations of the known High-Amplitude Delta Scuti star GSC 1374-01131 based on the Catalina Surveys publicly available data. ... From a single night of their observations, the variable was classified as a HADS (High-Amplitude Delta Scuti) star, with the light elements: . ... The light curves of GSC 1374-01131 based on Catalina data, folded with periods of pulsations and eclipses. ...

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• Journal "Peremennye Zvezdy" > PZ: main journal.
• Астронет > Англо-Русский Словарь

... 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| ...

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• http://www.sai.msu.su/gcvs/gcvs/nl75/readme

NMW survey overview . Access image archive . ... The New Milky Way survey aims to detect bright (V<13.5) optical transients near the Galactic plane using an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. ... All images obtained during the transient search survey are available online (please use the image archive access form ). ... Images per field: . ... Images per night: . ... Milky Way imaging time: . ...

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Электронная библиотека Попечительского совета . ... Harvey A.C. (ed.), Proietti T. (ed.) - Readings in Unobserved Components Models . ... Название: Readings in Unobserved Components Models . Авторы: Harvey A.C. (ed.), Proietti T. (ed.) . ... This volume presents a collection of readings which give the reader an idea of the nature and scope of unobserved components (UC) models and the methods used to deal with them. ... Электронная библиотека попечительского совета мехмата МГУ , 2004-2016 . ...

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• Good G.A. - Observing Variable Stars :: Электронная библиотека попечительского
• Milnor J. - Dynamics in One Complex Variable :: Электронная библиотека
• Freitaq - Several Complex Variables. Local Theory :: Электронная библиотека

New GCVS Version (GCVS5) FileName Explanations ----------------------------------------------------------------- ReadMe This file GCVS5 The ... ------------------------------------------------------ 1- 2 I2 --- Constell [1/88]Constellation numeric code 3- 6 I4 --- Number Star number within the constellation 7 A1 --- Component *Component identification 9- 18 A10 --- GCVS * Variable ... Field is non-blank if magMin is a magnitude or amplitude given in a system other than that indicated by magCode. ...

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• General Catalogue of Variable Stars: Vols I-III (the new electronic version).
• General Catalogue of Variable Stars: Variability Types
• General Catalogue of Variable Stars: Homepage.

... we show that the comparison between the calculated and observed numbers of the most ``fragile'' (from the point of view of the binary evolution scenario )   galactic binary types (such as X-ray low-mass X-ray binaries (LMXB), cataclysmic variables (CV),   Be-stars   with compact companions, relative number of visible binary radiopulsars   with normal and compact secondary components) impose certain constraints on the feasible initial ... Phenomenological Kick Velocity . ...

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• Seminars
• Sources in the LMC: comments to the Table 2
• Cyg X-3

... 2013 September 9 . Nearby Cepheid Variable RS Pup . Image Credit: Hubble Legacy Archive , NASA , ESA - Processing: Stephen Byrne . ... Pulsating RS Puppis , the brightest star in the image center, is some ten times more massive than our Sun and on average 15,000 times more luminous. In fact, RS Pup is a Cepheid type variable star , a class of stars whose brightness is used to estimate distances to nearby galaxies as one of the first steps in establishing the cosmic distance scale. ...

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• Bright Sn in NGC 3877
• Statistics from S. Pesci and P. Mazza logbook.
• Supernova 2000ch in NGC 3432

... There are preliminary series of photometric and radio spectral observations of the above-mentioned stars, archival data on the light curves of the stars, results of the search for OH and H 2 O maser emission in IRAS point sources that possess the IR parameters similar to Miras. ... The aim is a detailed study of the maser emission variability. ... In 1996-1997, astronomical observations of Mira Ceti-type stars (miras) were carried out in three spectral ranges: optical, infrared, and radio. ...

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• Rudnitskij Georgij M. Home Page
• Ссылки
• G. Rudnitskij's Links

PHP Manual . ... Variables . ... Sometimes it is convenient to be able to have variable variable names. ... In the above example, hello , can be used as the name of a variable by using two dollar signs. i.e. $$a = "world"; . At this point two variables have been defined and stored in the PHP symbol tree: $a with contents "hello" and $hello with contents "world". ... i.e. they both produce: hello world . In order to use variable variables with arrays, you have to resolve an ambiguity problem. ...

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• Variables from outside PHP
• Dealing with a Variable Number of Arguments/Optional Parameters
• Creating Variables

... The bright supernova (hereafter SN) in the galaxy NGC 4527 was first sighted by S. Knight (USA) on April 13.17UT at magnitude ~14.0v. The report of the sighting was subsequently forwarded by phone to the AAVSO. ... SN 1991T. The galaxy NGC 4527 is an Sb(s)II type galaxy with an apparent Blue magnitude of 11.32 (Shapley-Ames, 1981). ... An analysis of this event utilizing visual observations by amateurs, plus a light curve is presented.. ... THE LIGHT CURVE: . ... ISN SN 1991T web page . ...

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• Supernova 1999ee and 1999ex in IC 5179
• Supernova 2001ac in NGC 3504
• SN1989B in M66

... Другие названия журнала: Information Bulletin on Variable Stars , Information Bulletin on Variable Stars , I.B.V.S., показать полностью.. ... Stars , Information Bulletin on Variable Stars, . ... Prokhorov M.E. в журнале Information Bulletin on Variable Stars , издательство Konkoly Observatory (Hungary) , ? ... Kazarovets E.V. , Samus N.N. , Durlevich O.V., Kireeva N.N. , Pastukhova E.N. в журнале Information Bulletin on Variable Stars , издательство Konkoly Observatory (Hungary) , том 6052, с. 1-23...

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• Yudin B.F. - сотрудник | ИСТИНА - Интеллектуальная Система Тематического
• Complex Variables and Elliptic Equations - журнал | ИСТИНА - Интеллектуальная

. Alexey Rastorguev's software . Linsvd Linear least-square problem solution by singular value decompisition of matrix . Lafkin Periodogram calculation (Lafler-Kinman statistics) . FourierPeriodogram Periodogram calculation by Fourier-decomposition . Equ2gal Transformation of the equatorial coordinates and proper motions to the galactic frame . Galorbits.zip Calculation of orbits in three-component Milky Way galaxy model

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• Отдел Изучения Галактики и переменных звезд
• Yuri Nicolaevich Efremov - My Home Page
• Shugarov's Home Page

Geophysical Research Abstracts Volumi 3, 2001 . ... The observable lunar region was a seismic active region (30W, 5S). ... arcminutes long trip on the lunar surface in direction to Mare Serentatis. ... 23 Moon's phase angles and 1954 lunar regions. ... basin are compared to craters located in highland and mare regions. ... morphology of craters in the mare region is found to differ drastically from those in . ... and craters with faults in the mare region are due to lava flooding of ancient . ...

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Forming of landscape structure on south of Valday Hill M.Yu. ... Landscape components reflected through spatial variation of numerous properties, determined on digital elevation model (made with topographic map 1:100000), composition of multispectral images Landsat 5, Landsat 7, Geocover (1990 and 2000) and gridded maps of climatic variables with 10 arc minute resolution. ... Each landscape component has properties independent from the whole and determining its autonomous variation. ...

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• http://www.sevin.ru/ecosys_services/references/Puzachenko_Sankovski_Interrelation_factors_at_bioshere_level.pdf
• http://www.sevin.ru/ecosys_services/references/Kozlov_Identification_of_geosystems_formative_factors.pdf
• Экологический Форум - Фундаментальная Экология: replaceable hardware components

... public class ProtoVariable . ... ProtoVariable (java.lang.String name, java.lang.Class componentType, Dimension dimension) . ... If null or zero length array, this is a scalar variable. public ProtoVariable (java.lang.String name, java.lang.Class componentType, Dimension dimension) . ... dimension - A single dimension to define the array. public ProtoVariable (java.lang.String name, java.lang.Class componentType, Dimension [] dimArray, Attribute [] attrArray) . ... Returns the name of this Variable....

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• Client
• NetCDF User's Guide for C
• Appendix B File Format Specification

Search for Flavor Changing Neutral Currents in Single Top Quark Production -1 using 2. fb at D 3 Maxim Perfilov Moscow State University on behalf of the D0 Collaboration QFTHEP2010 , 2010 /09/14 Tevatron -396 ns between bunches - - has delivered about 9.2 fb since 2002 1 QFTHEP2010 , 2010 /09/14 2 FCNC models with soliton structure of the top quark Flavor Changing Neutral Currents change flavor of quarks without changing the charge models with ...

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Canidae . ... Analysis of variation of the cheek teeth in three canid species (Mammalia: Canidae) by means of standard and geometric morphometrics Zoological Museum of Moscow University Several methods of minimizing size from overall variation are compared, which are shape variables of geometric morphometrics, two methods of data standardization (by character means and by specimen centroids), and principal component analysis. ... Rohlf, 1986; Bookstein, 1991; Navarro et al., ... 414 Canidae . ... Vol. ...

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• http://zmmu.msu.ru/rjt/articles/ther8_2%20097_106%20Vinogradov.pdf
• http://zmmu.msu.ru/files/images/spec/Russ%20Ent%20J/ent19_1%20031_040%20(Tishechkin).pdf

... Let $(X_n)$ be a strictly stationary random sequence with the marginal distribution functions $F(x)=P{X_1\leq x}$. ... Let us denote $ M_n=\max {X_1,.. ... The limiting distributions of the random vector $(\tilde{M_n}, M_n)$ and "asymptotic independency" of $\tilde{M_n}$ and $M_n$ are obtained under some condition of weak dependency of random variables from sequence $(X_n)$, which is more restrictive than Leadbetter's $D(u_n)$ condition, and some conditions on the sequence $(\varepsilon_n)$. ...

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The user phase space function has a prototype . double usrfun(char * name) . ... is called for the user input of the structure function parameters just after the particular structure function is chosen. ... In the simplest case, if the user would like to implement a new structure function without singularity and extra parameters, he may take a copy of the $COMPHEP/c_source/num/strfun/sf_prv.c file, improve p_prv so that it returns in any case, and rewrite the originally trivial c_prv function. ...

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• [RU-NGI] Fwd: [Inspire-sa1] last glite 3.1 components in staged rollout
• [RU-NGI] Fwd: [Inspire-sa1] reminder: gLite 3.1 components reaching end of
• The genEvents command

... 2 ftp://ftp.ebi.ac.uk/pub/databases/rcsb/pdb/data/monomers/components.cif.gz . 3 codes_py = allpy/data/codes.py . 4 components_cif = allpy/data/components.cif . ... 6 all: doc codes tests . ... 11 doc: . 12 sphinx-autopackage --suffix = rst --dest-dir = docs/source/allpy/ allpy . 13 $( MAKE ) -C docs html . ... 15 force-doc: . 16 rm docs/source/allpy/* . 17 rm -rf docs/build . 18 $( MAKE ) doc . ... 20 codes: $( codes_py ) . ... 26 $( codes_py ) : $( components_cif ) . ...

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• allpy: Makefile annotate
• allpy: b5a5f46a48a7 Makefile
• allpy: 6faac45a3a17 Makefile