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1. Detection rate of binary compact star merging
Next: Discussion Up: No Title Previous: Parameters of binary compact . Under the assumptions made above, we can calculate the binary merging rates in the Galaxy R . ... Figure: The dependence of different compact binary merging rates in a model ``elliptical'' galaxy (where all the stars were formed simultaneously at the moment t =0) with mass M . The horizontal line shows the mean merging rate of binary NS in a spiral galaxy of the same mass with a stationary star formation. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~lipunov/kionewht/node10.html -- 9.8 Кб -- 16.06.2000
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2. (Untitled)
The data in the Table on p. 5788 – 5789 embrace estimated parameters for 128 binary systems in near Earth, Mars crossing, main belt and Trojan orbits (more than 90% of corresponding objects are marked in the Table "Minor planet lightcurve parameters" as undoubtedly binary and in other cases as suspected binary). ... The data were presented by P. Pravec (Astronomical Institute, Academy of Sciences of Czech Republic) (see Pravec, P., Harris, A. W., 2007. Binary Asteroid Population. ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user9gs2.htm -- 2.3 Кб -- 10.04.2016
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3. White Dwarf Merger Movie
Hideyuki Saio Simon Jeffery are exploring models for the evolution of stars formed by the merger of two white dwarfs. The attached movie provides a simulation of the major events involved in the merger process. ... An initial binary system consists of two white dwarfs of masses M 1 and M 2 (given) with an orbital period ( P ). ... We adopt a simple expression for the white dwarf radius as a function of mass (in solar units): . ... The merged star evolution is simulated by a quadratic expansion . ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~csj/movies/merger.html -- 8.3 Кб -- 08.08.2001
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4. http://xmm.vilspa.esa.es/sas/7.1.0/doc/merge/ChangeLog
... SPR-2608) Version 0.11 - 2003-12-02 (HB) ----------------------------------- + ( src / merge_mod.f90 ): TSTOP keyword was not updated correctly; fixed. closed SPR: + SSC-SPR-3158: merge does not update the TSTOP keyword Version 0.10 - 2003-05-07 (HB) ----------------------------------- + (config/ merge .par): modified to enable param-2.0 functionality Version 0.9 - 2003-04-04 (HB) ----------------------------------- + ( doc / ... Just to reiterate, do take care with any merged output. ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/7.1.0/doc/merge/ChangeLog -- 5.3 Кб -- 10.01.2007
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5. The main observational parameters
... Column 1 gives the object name from the Case or Markarian catalogs. ... For Markarian galaxies the errors of coordinates usually lie inside 2'' (Lipovetsky [ 1983 ]). Column 4 gives the eye-estimated apparent blue magnitudes according to the same sources. ... Other names of a galaxy we give in column 7. ... In column 3 we cite the original emission-line code of the galaxy for the strength of [O III ] doublet according to the Case catalog (s - strong, m - medium, w - weak). ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Laboratory/Publications/1997/CasePR/node7.html -- 10.4 Кб -- 10.01.1998
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6. The Space Science Case for
Prof. Mike Kelley recently asked for a meeting with Cornell President David Skorton, a meeting which subsequently occurred on Monday, August 27, to discuss the Arecibo situation from a near earth space science perspective. ... On the importance of the Arecibo Observatory (AO) to near Earth Space Science, both Space Weather and Near Earth Asteroid/Planetary Studies, at Cornell University?the non-(classical) Astronomy Faculty . ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/aorss/space_science.html -- 4.6 Кб -- 29.07.2008
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7. Plots for Estimating Point Source SNR
In this section we present plots which may be used to rapidly estimate signal-to-noise ratio (SNR) for point sources with stellar spectra observed through popular WFPC2 filters. ... Dotted lines across the top of each plot indicate the onset of saturation. ... We look at Figure A2.10 and find this value on the horizontal axis. ... This exposure is well below the saturation lines in the plot, so saturation is not a concern. ... 0.45 Figure A2.1: Point Source SNR vs. V+AB for F160BW Filter. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/instruments/wfpc2/Wfpc2_hand2/ch999_appendix_b_snr2.html -- 30.9 Кб -- 29.08.2000
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8. astro-ph authors/title/abstract search for 'galaxy merging' all years
... Authors: Spyros Basilakos (Imperial College London) . ... Title: Populating a cluster of galaxies - I. Results at z=0 . ... Title: The Merger Rate to Redshift One from Kinematic Pairs: Caltech Faint Galaxy Redshift Survey XI . ... Title: Multi-wavelength observations of an evolved galaxy group: An endpoint of galaxy merging? ... 23 matches for the search pattern galaxy merging . The URL for this page is: http://xxx.itep.ru/find/astro-ph/1/galaxy+merging/0/1/0/past,all/0/0 www-admin@xxx.lanl.gov ...
[ Сохраненная копия ]  Ссылки http://sed.sao.ru/lit/gal_merg.html -- 19.7 Кб -- 15.07.2001
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9. Astronomy HyperText Book: Stellar Clusters
Stellar Clusters are very useful laboratories for empirically studying stellar evolution. ... All cluster stars are at the same distance . All cluster stars have the same physical age . ... CM diagram Young Cluster In this case we see the Main Sequence fully represented. The blue dots represent massive stars with short main sequence lifetimes. ... Thus, identifying the most massive star which is still on the main sequence is an effective means of determining the age of a stellar cluster. ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/textbook/sc.html -- 3.5 Кб -- 23.01.1998
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10. Configuration Options
... In some cases where memory space is at a premium, it is possible to tailor the configuration to remove such features as reference clock driver support, debugging support, and so forth. ... The following lines are used in this file: . ... The DEFS_LOCAL line defines global flags that apply to all machines. Ordinarily, the only flags included are the -DDEBUG , which includes the debugging code, and -DREFCLOCK , which includes basic reference clock support. ... D_INCLUDE_BSD_SOURCE . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/~er/xntp/config.html -- 8.1 Кб -- 21.12.2007
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11. Untitled Document
... Unsafe act - a behavioral departure from an accepted, normal, or correct procedure or practice which, in the past, has produced injury or property damage or which has potential for doing so in the future; an unnecessary exposure to a hazard; conduct reducing the degree or safety normally present in an activity. ... Any hazardous unsafe condition, or act that presents a situation of imminent danger to life and/or property requires urgent action. ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Site/usersguide/SafetyPlan/06SafeSec3.html -- 4.9 Кб -- 20.05.2009
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12. The sculpture presented to John Anderson
... The Launch of "Stromlo, an Australian ObтАж . The sculpture presented to John Anderson . Sidebar Left . Sidebar Top . No Sidebar . ... Title: The sculpture presented to John Anderson . Description: The glass is a fragment of a flint glass lens and the base is a melted aluminium crucible. The plate was inscribed "Stromlo Observatory 2003". ... The sculpture presented to John Anderson The glass is a fragment of a flint glass lens and the base is a melted aluminium crucible. ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/gallery3/index.php/first100years/album26/IMGP4559 -- 21.9 Кб -- 10.04.2016
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13. Control statements
As conditional or control statements you have IF in many variants (but essentially not changed from Fortran 77), DO (with some new variants) and the completely new statement CASE . The DO- loop should now be ended with the statement END DO and we no longer need any statement number. In addition, we can use the statement EXIT to jump out of the DO -loop and CYCLE in order to go to the next iteration of the present DO -loop. ... all negative numbers WRITE (*,*) 'Negative number' CASE (0) ! ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/f77to90/c6.html -- 5.4 Кб -- 17.02.1996
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/f90/c6.html -- 5.4 Кб -- 17.02.1996
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14. Identification and Analysis of Binary Star Systems using Probability Theory
... Accurate identification of physical binary star systems has become of increasing interest in recent years. ... Identification of physical binary star systems, with an estimated reliability of such identifications based on the theory of probability, is also important for current and future efforts to find binary star systems that are candidates for observations with the aim of determining their orbits and component masses. ... probability of the proximity of proper motions and ; . ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/grochevae.html -- 17.6 Кб -- 12.06.2006
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass97/grochevae.html -- 17.6 Кб -- 15.05.1998
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15. II-VI compound crystal growth, HPVB & HPVZM basics
II-VI compound crystal growth, HPVB & HPVZM basics . ... Developed and first time applied for II-VI compound crystal growth in our lab back in late sixties [1]. ... Basics . The II-VI compounds have particular physical-chemical properties that present a challenge for the crystal growth. ... In the general case of II-VI compounds and HPVB growth conditions: . ... These peculiarities of composition stipulate another problem of the II-VI compound crystal growth from the melt - "bubbles". ...
[ Сохраненная копия ]  Ссылки http://www.issp.ac.ru/lpcbc/Basics.html -- 9.3 Кб -- 16.03.2004
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16. Ya.B. Zeldovich All-Moscow Seminar of Astrophysicists
... Seminar archive . ... Титарчук Л. X-ray spectral index correlations vs mass accretion rate in neutron star and black hole X-ray binaries in their different spectral states. ... vs mass accretion rate as in the case of NS as well in the BH case. In BHs the spectral index should increase and then saturate with mass accretion . ... BH case the index, indeed, correlates and then saturates with mass accretion . rate. Moreover this index-mass accretion rate correlation allows us to estimate . ...
[ Сохраненная копия ]  Ссылки http://master.sai.msu.ru/en/osa/archive/2016/03/18/ -- 7.8 Кб -- 09.04.2016
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17. The Present and Future of Small and Medium Size Telescopes
. English / Russian . Conference . Committees . Registration . Abstracts . Program . Venue . Accommodation . Contacts . Send your application and Abstract by e-mail to: smt-conf@sao.ru until 20 august 2015. The application form should include . Full name . Organization . Title of your presentation . Your application will be confirmed by e-mail . 2015 SAO RAS
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/lon/ConfSite/thesis-en.html -- 3.0 Кб -- 10.04.2016
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/lon/ConfSite/thesis-en.html -- 3.0 Кб -- 10.04.2016
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18. http://www.mrao.cam.ac.uk/~bn204/mk2/publications/2005/abs_thesis.html
... OOF . ... OOF Index . ... Title: Nuclear Starbursts Abstract: Investigations of some aspects of star formation in external galaxies are presented. ... Emphasis is placed on interpretation of mid-infrared observations, and as an important tool for this, a comprehensive and physical model for dust emission from nuclear starbursts is developed. \vspace*{0.5cm} It has been shown that galaxies with close companions have star-formation rates which are, on average, enhanced compared to isolated galaxies. ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/mk2/publications/2005/abs_thesis.html -- 9.5 Кб -- 25.11.2009
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19. Sheltran - SELECT construct
SELECT <arithmetic expression> CASE n1 [,n2...] [ <statement>.. ... OTHER [ <statement>.. CSELECT . ... At least one integer must be present for each CASE statement. the integer values may appear in any order in the CASE clause. the CASE clauses need not contain all values in the range 1 to N, where N is the largest integer value used. ... SELECT COLOR+1.0 CASE 1 COLTXT='BLACK' CASE 2 COLTXT='RED' CASE 3 COLTXT='GREEN' CASE 5 COLTXT='BLUE' CASE 8 COLTXT='WHITE' OTHER COLTXT='MIXTURE' CSELECT . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/gipsy/sheltran/SELECT.html -- 2.7 Кб -- 16.01.2009
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20. Case чувствительность (чувствительность к выбору)
... Вы можете, например, написать TITLE , или Title , или title , или даже tItLE, если Вам нравится. ... Но существуют и case чувствительные конструкции языка, а именно: . ... URL , так как он может содержать наименования файлов, которые являются case чувствительными во многих операционных системах (например, в Unix). ... Что касается синтаксиса URL, смотрите ftp://ftp.funet.fi/pub/doc/rfc/rfc1738.txt (полные URL записи) и ftp://ftp.funet.fi/pub/doc/rfc/rfc1808.txt (относительные URL записи). ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/vch/RusDoc/html3.2ex/gl_11.htm -- 4.0 Кб -- 17.03.1998
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/vch/RusDoc/html3.2ex/gl_11.htm -- 4.0 Кб -- 17.03.1998
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/vch/RusDoc/html3.2ex/gl_11.htm -- 4.0 Кб -- 17.03.1998
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