Next: Star Formation Rate and Up: No Title Previous: Calculation of Evolutionary Tracks . To start calculations, we choose the distributions of the initial binary parameters: the mass of the primary ZAMS component, , binary mass ratio, , orbital separation a . ... whereas the mass ratio distribution is not. ... The zero assumption often made is that the mass ratio distribution has a flat shape, that is binaries with a high mass ratio occur as frequently as those with equal masses. ...

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• Test of the Initial Mass-Ratio Distribution
• Amplitude Distribution
• Dependence on the Scenario Parameters and Initial Distributions

... Species distribution . ... According to Pfam database there have been found 487 ETS genes to date, most of which turned out to belong to different species of animal kingdom. ... The following table shows the number of ETS genes present in genomes of most intensively studied species. The number of ETS genes found in genomes of most intensively studied species . ... The following table shows the number of well studied ETS proteins and their distribution among species. ... ETS1, SPI1, SPIB . ...

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• HTH3_species_distribution

. Supernovae distribution according to their magnitudes. This graph shows the distribution of SNe according to the magnitude. This graph is kept up to date till SN 2000ek . Along X-axis there are all magnitudes bands so that you have to read in this way: for example, the band on the graph marked as 18 takes in all supernovae between mag.17 and 18, or if one prefers ...until less than mag. 18, and so on...

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• Distribution of Supernovae according to their parent galaxies' recession
• Distribution of Supernovae according to their parent galaxies' morphological
• APOD: 2007 May 29 - Bright Spiral Galaxy M81 from Hubble

by Margarita Dzhalalova It is known that the pressure difference values for a round parachute are constant over total canopy, then for a square parachute the values of pressure difference are non-uniform along radial ribbons differing even from each other and depending mainly on certain sets of line lengths, and therefore square parachutes attain different shapes from each other ( Fig.1 - photo of var.1 and var.2). ... Distribution of pressure coefficient along radial ribbons of square parachute. ...

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• Scientific Achievements

This page is devoted to information on Supernova 1999gn in NGC 4303 (= M61 ) Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main supernova page. Information on the original web pages for many of these images can be found on the Supernova links web page. ... SEDS has a Supernova 1999gn page . ... Seiichi Yoshida has a 1999gn page . ... Kopernik 's M61 and supernova 1999gn page . ... vsnet-alert 3835 ] SN 1999gn in NGC 4303 = Messier 61 . ...

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• THE BRIGHT SUPERNOVA 1991T IN NGC 4527; AN AMATEURS PRESPECTIVE
• Nova in M31 2000 3
• SN1989B in M66

Microsymposium 38, MS083, 2003 (A4 format) MERCURY: LOCAL VARIATIONS OF THE PHOTOMETRIC RELIEF. ... Because of trajectory and pointing angle constraints the planet could be observed from Mariner 10 only over a small range of phase angles between about 75o and 110o. Therefore the photometric investigations are restricted to measuring the distribution of brightness on the Mercurian disk. ... Raw versions of real-time processing pictures FDS 0000984 and FDS 0000986 were used (images 196 and 202). ...

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• http://selena.sai.msu.ru/Bus/Publications/m44_14_busarev_etal.pdf
• http://selena.sai.msu.ru/Pug/Publications/Pugacheva%20LPS%2041.pdf
• http://selena.sai.msu.ru/Shev/Publications/m44_76_sinitsin_shevchenko.pdf

... J.K. Krylov . In the monography by R. Koehler [1] there was described a very interesting effect of the words' average length oscillation as a function of their frequency of use (according to the data from a representative frequency dictionary). ... In this context, further the Koehler's effect will be definied as polymodal character of the dependence of the conditioned average in cases of two-dimencional distributions of any linguistic nature. ...

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• MSU-LGCLL:: Krylov J.K.- Three Laws of Fiction Prosaic Texts Organization

... The main field of my investigations is stellar spectrophotometry. As a result of scientific activity of our group spectrophotometric catalog was created including energy distribution data on 900 stars in the range 3200-7600AA and 250 stars in the range 6000-10800AA (Voloshina et al., Spectrophotometry of Bright Stars, ed. I.N.Glushneva, 1982, Moscow, Nauka, in Russian). ...

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... Seares F.H., van Rhijn P.J. - Distribution of the Stars with Respect to Brightness and Distance from the Milky Way . ... Название: Distribution of the Stars with Respect to Brightness and Distance from the Milky Way . Авторы: Seares F.H., van Rhijn P.J. Язык: . ...

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• Brown E.W. - An Explanation of the Gaps in the Distribution of the Asteroids
• Klyshko D.N. - Photons and nonlinear optics :: Электронная библиотека
• von Collani E., Drager K. - Binomial Distribution Handbook for Scientists and

New RRC variables with an additional non-radial pulsation . PZ, vol. ... We present a new study of 14 known RR Lyrae variable stars from the Catalina surveys periodic variable star catalog. ... New Double-Mode RR Lyrae Variables III . ... We present a new study of 123 known RR Lyrae variable stars from the Catalina surveys periodic variable star catalog. ... According to these data, the stars are double-mode RR Lyrae variables, pulsating in the first-overtone and fundamental modes. ...

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• Milky Way Illustrated
• Journal "Peremennye Zvezdy"
• Астронет > Milky Way Illustrated

... For SUSY this quantum numb er is R-parity, for IDM that is sp ecific D-parity 2 Most probable: Dark matter particle is neutral D0, Mass < 60 - 70 GeV,(to prevent annihilation D0D0 W +W - even slightly b elow threshold) The charged particles having the same quantum numb er DБ are heavier than 100 GeV (LEP), In the scalar case the counterpart with opp osite P-parity DA also exists, they are lighter than ab out 120 GeV(LEP). ... Their cross sections contains additional factor - two orders lower. ...

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... One of the most widely used tools of Fourier analysis is the Parseval theorem. It enables the experimentalist to view how the `energy' in the signal is distributed among frequencies. The Fast Fourier Transform (FFT) algorithms have made power spectra one of the obvious diagnostics tools during data acquisition, and energy maps are a versatile alternative. ... The result is an energy map (Fig. 9), showing the distribution of energy corresponding to the wavelet map (Fig. ...