... If the parameter withinputlist is set to ``true'', the reconstruction and/or background image will be created using source parameters from an input source list. ... Use parameters makerecon and savebkgrnd to specify which of the output images you want to create. Only sources originally detected at scales up to maxscale will be used for to calculate the images. The value of maxscale will also control the scale of the kernel used to filter the background image. ...

Laboratory of Stellar Physics . ... A study of close binaries with black holes, neutron stars and white dwarfs. ... A study of SS433 - the massive close binary with a black hole in the regime of supercritical accretion . ... A search for intermediate-mass black holes (IMBH). The black holes which are not supermassive black holes observed in quasars, and which were formed not in massive stars. ... A search for new magnetic stars, new CP stars, measurements of magnetic fields in stars . ...

... Aurora from Space . ... Magnetic Storms . ... The "ring of fire" seen by satellite cameras around the polar caps (picture below) is probably created by electrons leaking from the tail's plasma sheet, whose magnetic field lines form a somewhat imperfect trap. ... One possible explanation involves the close association between auroral arcs and electric currents which flow along field lines between the ionosphere and distant space ( Birkeland currents ). ... Why no aurora at the magnetic poles? ...

... This program was created for correlating chosen regions in the series of fts images. ... Chosen regions' . ... In this section the program counts the integral for each region of the grid for each image. ... As a matter of fact, the integral is total brightness of the region and it is counted by 'int_tabulated' IDL function. ... In addition, the program will show the count of the regions which correlate with the corresponding region (the brighter region means the bigger count) and its contour. ...

The database contains references to the papers, data files and links to the Internet resources related to measurements and calculations of the optical constants in the wavelength interval from X-rays to radio domain. ... References to some useful books and reviews on the subject (e.g. the classical handbooks edited by E.D.Palik) and links to Internet collections of optical constants and personal WWW pages with related software were also placed in the database. You have arrived at our welcome page. ...

One of the most important questions in astronomy today is the source of the ionising photons that caused a predominantly neutral Early Universe to evolve into the ionised one we see today. ... Although the global star formation history of the early universe is strongly constrained by current observations, we actually know little about the nature of star formation at this time (as given by the specific star formation rate). ...

home publications > mercury . ... Rings of Creation . ... In 1755, Immanuel Kant had the remarkable insight that stars and planetary systems form by the gravitational collapse and rotational flattening of interstellar clouds. Later in the 18th century, Marquis Pierre Simon de Laplace refined Kant s idea by suggesting that planets condensed from rings produced at the edge of a contracting disk while the Sun formed at the center a picture thereafter known as the Nebular Hypothesis. ...

... Suppose we have 2 tones Acos(at) and Bcos(bt). ... The individual freq terms are then: . ... square :[Acos(at) + Bcos(bt)]^2: [Acos(at)]^2 +[Bcos(bt)]^2 + 2ABcos(at)cos(bt) . ... A^2(cos(2at) -1)/2 . ... A^3cos(at)*[cos2at - 1)/2=A^3([cos(3at) + cos(at)]/2 - cos(at)]/2=A^3(cos(3at) -cos(at))/4 . B^3cos(bt)*[cos2bt - 1)/2=B^3([cos(3bt) + cos(bt)]/2 - cos(bt)]/2=B^3(cos(3bt) -cos(bt))/4 . let C2= 3AB^2 and C3=3BA^2 . ... C 3cos(bt)[cos(2at)-1]/2=C3[{cos((2a-b)t)+cos((2a+b)t)}/2+cos(bt)]/2 . ...

... Submitted by Al Takeda on 12/24/2012 23:40:10 . Large Magellanic Cloud (LMC) . The larger of the 2 Magellanic Clouds, this dwarf galaxy spans an area of 650-minutes x 550-minutes (10-degrees) and is 160,000 light years away on the border of the constellations of Dorado and Mensa. ... The LMC was the host galaxy to supernova 1987A. 7 images x 27-second subframes, Total= 3 minutes 9-seconds. ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

... PDF created with pdfFactory Pro trial version www.pdffactory.com .1 (LOD) (M>6) XX . ... PDF created with pdfFactory Pro trial version www.pdffactory.com , , , . ... http://www.iris.washington.edu/] DMS IRIS, 318 >4 1964 2000 300 5 . ... M > 5.5 M < 5.5 . ... Geophysical Res. ... Evolutionary features of the geophysical time series: -I. Tide process and seismic series V.M.Vorotkov, V.L.Gorshkov Summary The new method of comparative study of the geophysical data of a various nature is offered. ...

A great many years ago, one of our members created a type of slide show that took you on a guided tour of Warren Rupp Observatory. Needless to say, that was a great many years ago and things have changed for the better! ... Warren Rupp Observatory is proud to be associated with these fine groups and endorse these resources.. ... The WRO/RAS was designed and donated by Tammy Plotner - Copyright 2008-2015; Original Content - Tammy Plotner - Copyright 2008-2015; All rights reserved. ...

Next: Binary Radiopulsars with Black Up: Black Holes in Binaries Previous: Black Holes in Binaries . Two different types of stellar BH formation exist: (1) direct core collapse   of a massive star and (2) AIC of a NS. A BH of the first type presumably will have a mass comparable to that of the collapsing star and can be born both from a single star and in a binary system. ... Next: Binary Radiopulsars with Black Up: Black Holes in Binaries Previous: Black Holes in Binaries Mike E. Prokhorov . ...

NAME htdigest - Create and update user authentication files SYNOPSIS htdigest [ - c ] passwdfile realm username DESCRIPTION htdigest is used to create and update the flat-files used to store usernames, realm and password for digest authentica- tion of HTTP users. Resources available from the httpd Apache web server can be restricted to just the users listed in the files created by htdigest. This manual page only lists the command line arguments. ... OPTIONS -c Create the passwdfile . ...

. The telescope was reassembled over the past few days and stands ready for the windscreen. I have created two site for these pictures: one with small image sizes, the other with larger image sizes. This is the larger image size file. Captions above photo . The following are different views of the assembled telescope. A big thanks to French Leger and Larry Carey, both from UW. Photos taken by Gretchen Van Doren/APO.

... Бренд: Zapf Creation, Тип: Колготки для кукол . Аксессуары для кукол . ... Пособие содержит темы, подготовленные на основе базовой учебной программы по дисциплине "Банковский маркетинг". ...

... In spite of the lack of rich clusters around us and the presence of large volumes completely free from galaxies (voids), the mean luminosity densities and the mean density of hydrogen mass in the Local Universe is one and a half - twice as high as their mean global values. However, the mean local density of the baryon mass is only 2% of the critical density of the Universe, which is twice as less as the baryon density from the nucleosynthesis data (local paradox of the baryon mass). ...

OptInt PmWiki : Pm Wiki / Creating New Pages . ... Links > . ... The first step to create a new page, you need to edit an existing page, and on it add a link to the page you want to create. To link to your new page, you must choose a name for it. ... Typing [[my new page]] will create a link to my new page ? ... PmWiki will then dutifully tell you that the page you entered doesn't exist, but you can click on the "Edit" link in order to create, edit, and save the new page. ...

... Class . ... Tree . ... Creates a panel with the hierarchical tree structure of (some of the) ImageJ's commands according to the structure of the String argument (see below). int[] . ... imagej menus" . creates a tree with all of ImageJ's menu structure, that means it replicates in tree form the ImageJ's menu bar; this includes any jar plugin and user plugins . ... Please note that when no arguments are passed, ImageJ's menus will be shown as a unique tree named "Control Panel"; if "imagej menus" . ...

Abstract -- Calculations are performed for the circular polarization of maser radiation from a turbulent, Keplerian disk that is intended to represent the sub-parsec disk at the nucleus of the galaxy NGC4258. ... This turbulence, along with the Keplerian velocity gradients and the blending of the three hyperfine components to form the 6 16 --5 32 masing transition of water, are key ingredients in determining the appearance of the polarized spectra that are calculated. ...

... 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). ...