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http://www.sao.ru/Doc-en/SciNews/2010/CHCyg/.

1. CH Cyg
... The hot component shows very spectacular activity: irregular outbursts accompanied by fast, massive outflows and jets. ... Diffraction-limited images for both components of CH Cyg binary system were reconstructed using visible speckle interferometry at BTA 6-m telescope (Fig.1). The orbital period 15.6 years and masses: 2.0 Msun and 0.7 Msun for red giant and white dwarf, respectively were derived from angular distance (0.042") and magnitude difference (2 m ) of the components. ... Fig.1. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/Doc-en/SciNews/2010/CHCyg/ -- 4.2 Кб -- 02.10.2012
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/Doc-en/SciNews/2010/CHCyg/ -- 4.2 Кб -- 02.10.2012
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2. http://www.mrao.cam.ac.uk/~anthony/latex/Norbury.ps
A New Mass Model For The JVAS Gravitational Lens B1030+074. ... University of Manchester, Jodrell Bank, U.K. B1030+074 is a double image gravitational lens, which was dis- covered during the Jodrell Bank VLA Astrometric Survey (JVAS). ... HST WFPC2 observations have revealed the lensing galaxy, which lies close to component B. The redshifts of the lensing galaxy and the background source have also been obtained and are 0.599 and 1.535 respectively. ...
[ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~anthony/latex/Norbury.ps -- 27.3 Кб -- 24.06.2000
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3. Results
... We have been using it to analyze PC images of known gravitational lenses and QSOs which are candidates for lensing (Falco 1993). ... Fig. 1 plots the higher contours of the PC image of 0142 in the upper left, and its power spectrum in the upper right. ... If we fit the envelope of the power spectrum with a binary model, we find that best fit gives a separation of the two components of 1.3 PC pixels or about 58 mas. ... The lower two curves are cuts through the 0142 power spectrum. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/irw/proceedings/nisensonp.dir/section3_3.html -- 7.5 Кб -- 16.04.1994
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4. casacore: components/ComponentModels.h Source File
... Modules . ... Classes . Files . ... File List . File Members . components . ... National Radio Astronomy Observatory 00023 //# 520 Edgemont Road 00024 //# Charlottesville, VA 22903-2475 USA 00025 //# 00026 //# $Id: ComponentModels.h 20691 2009-07-14 03:13:54Z Malte.Marquarding $ 00027 00028 #ifndef COMPONENTS _ COMPONENTMODELS _H 00029 #define COMPONENTS _ COMPONENTMODELS _H 00030 00031 # include components / ComponentModels /ComponentType.h 00032 00033 # include components / ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/casacore/casacore-1.2.0/doc/html/ComponentModels_8h_source.html -- 18.4 Кб -- 14.02.2011
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5. ContrastAdjuster (ImageJ API)
... Class . ... METHOD . ... java.lang.Object java.awt.Component java.awt.Container java.awt.Window java.awt.Frame ij.plugin.frame.PlugInFrame ij.plugin.frame.ContrastAdjuster . ... public class ContrastAdjuster . ... Nested classes/interfaces inherited from class java.awt.Frame . ... Nested classes/interfaces inherited from class java.awt.Window . ... Nested classes/interfaces inherited from class java.awt.Container . ... Nested classes/interfaces inherited from class java.awt.Component . ... void . ...
[ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/software/astroimagej/imagej/api/ij/plugin/frame/ContrastAdjuster.html -- 32.1 Кб -- 02.12.2010
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6. Armagh Observatory
... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Sample fits to the SB2 observations of HD 22128 (top two frames) and HD 56495 (bottom two frames). Fits (smooth lines) to the observations (points) show the combined synthetic spectra, as well as the two component synthetic spectra. ... HD 22128 and HD 56495 are both double-lined spectroscopic binary systems with short orbital periods, which have been proposed to host magnetic Ap stars. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/highlights/2013/635.html -- 6.0 Кб -- 12.06.2013
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7. Journal "Peremennye Zvezdy"
Peremennye Zvezdy", . ... Star Name: . GSC 3710-00312, USNO-A2.0 1425-04252279 . ... Variability type: . ... USNO-A2.0 1425-04252279 is located at the distance of 15?.7 from the X-ray source 1RXS J031707.9+572942, which is larger than the position error of the source (12?), but its hardness ratio HR1 = 0.03 0.29, typical of chromospherically active stars, and its character of variability allow us to assume that the star is related to the X-ray source. ... Eclipsing variability . Sine wave 1 . ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/varstars/msg/1250291 -- 11.7 Кб -- 03.02.2013
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8. APOD: 2003 March 23 - Alpha Centauri: The Closest Star System
... 2003 March 23 . Alpha Centauri: The Closest Star System . ... Explanation: The closest star system to the Sun is the Alpha Centauri system . ... The bright stars Alpha Centauri A and B form a close binary as they are separated by only 23 times the Earth- Sun distance - slightly greater than the distance between Uranus and the Sun . ... By an exciting coincidence, Alpha Centauri A is the same type of star as our Sun , causing many to speculate that it might contain planets that harbor life. ...
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