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http://hea.iki.rssi.ru/conf/hea2010/Presentations/24/Titarchuk.pdf.
http://hea.iki.rssi.ru/conf/hea2010/Presentations/24/Titarchuk.pdf.
1. Number of accreting X-ray binaries of selected types
... The numbers of three types of compact binaries containing accreting NSs and BHs, which are most interesting from the point of view of their observational appearances, have been calculated as a function of time: i) X-ray transient source containing a NS in an eccentric orbit around a main sequence Be-star (the observed prototype: A0535+26), ii) BH The evolution of the selected types of X-ray binaries during the first 10 million years after the starburst onset is presented in Fig. ...
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Ссылки http://xray.sai.msu.ru/~polar/html/publications/apj/node8.html -- 5.9 Кб -- 21.06.1996
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2. http://www.iki.rssi.ru/seminar/20100609_11/Krivosheyev.pdf
... Moscow, Russia E-mail: krivosheev@iki.rssi.ru Notes: · · The Monte Carlo method (s) is also called the statistical test method An innumerable number of processes can be listed the outcome of which is not determined and has probabilistic nature, but these processes obey statistical laws, so to obtain the result we have to make multiple similar tests, i.e. to use the MC method Because probabilistic processes are widely spread in nature, the MC ...
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Ссылки http://www.iki.rssi.ru/seminar/20100609_11/Krivosheyev.pdf -- 663.0 Кб -- 29.06.2010
[ Текст ] Ссылки http://www.cosmos.ru/seminar/20100609_11/Krivosheyev.pdf -- 663.0 Кб -- 29.06.2010
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[ Текст ] Ссылки http://www.cosmos.ru/seminar/20100609_11/Krivosheyev.pdf -- 663.0 Кб -- 29.06.2010
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3. IAJ: Contents - Volume 23 Number 2
CONTENTS Volume 23 Number 2 (July 1996) . ... ENVIRONMENTS OF ACTIVE CLOSE BINARY STARS . A. G. Gunn . ... K-BAND OBSERVATIONS OF THE FLARE STAR UV CET . A. D. Andrews & P. M. Panagi . ... Elma S. Parsamian & A. D. Andrews . ... ASTRONOMICAL CLOCKS AT ARMAGH OBSERVATORY . ... JOHN BIRMINGHAM ON ``COGGIA'S COMET. ... 1995-1999 Irish Astronomical Journal, Downshay, 12 Heather Lea Avenue, Dore, Sheffield S17 3DJ, S. Yorkshire, United Kingdom WWW Contact: Alastair G Gunn Back to IAJ Home Page ...
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Ссылки http://star.arm.ac.uk/iaj/online/vol23no2.html -- 3.4 Кб -- 15.10.1998
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4. Procedure for Part Numbering Convention: Larry Carey, 2005
Numbering Procedures for APO 2.5m and 3.5m Drawings and Engineering/Drafting Documents . ... Document part numbers are to consist of a 7 character long "base numbe,r" which is coded to provide information about the part's intended first use. The part number becomes complete and unique only with the addition of a revision number. ... Example of a "base number": 25CSA01 . ... PART NUMBER CONVENTION . ... For Example: . ... R = "Revision" . ... Questions contact Larry Carey/University of Washington ...
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Ссылки http://www.apo.nmsu.edu/Telescopes/06APODrawNumConv.htm -- 8.3 Кб -- 22.03.2006
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5. Red synchrotron jets in Parkes quasars
We present model fits to spectral energy distributions in the optical and NIR of >100 flat-spectrum radio quasars from the Parkes Half-Jansky Flat-spectrum Sample. We find that ~40% of the sources have power-law SEDs, while a similar number show evidence for two primary components: a blue power law and optical synchrotron emission. ... The sources with power law SEDs show evidence for an excess number of red power law slopes compared to optically-selected quasars. ...
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Ссылки http://www.atnf.csiro.au/people/Matthew.Whiting/papers/html_abstracts/red_quasars_abs.html -- 3.8 Кб -- 26.12.2007
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6. Extended time series of Solar Activity Indices
Extended time series of Solar Activity Indices (ESAI) is database including observational, synthetic and simulated sets to study Solar magnetic field variations and their influence on the Earth. ESAI extend the ordinary lengths of some traditional indices of solar activity: sunspot areas, Wolf numbers (equatorial component of magnetic field of the Sun), polar faculae numbers (polar component), mean latitudes, N-S asymmetry of hemispheres (location of activity). Series . ...
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Ссылки http://www.gao.spb.ru/database/esai/readme.html -- 5.0 Кб -- 21.05.2007
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7. http://www.iki.rssi.ru/galeev/astro2007/krivosheyev2007.pdf
... Mass ratio of SS433 components is q = M X / MV = 0.2 В 0.3 . ... The spectum corresponds to precessional moment T3, i.e. when the angle between jet axis and the line of sight is equal 60 degrees. 10 -2 10 -3 lg I, phot/cm2/sec/keV 10 -4 10 -5 10 100 lg h, keV Cherepashchuk A.M.,Sunyaev R.A., Fabrika S.N., Postnov K.A. et al./ ... 5 10 100 Tcor = 20keV lg h, keV Mjet = 21020 g / s Lk = 61039 erg / s Angle dependence of SS433 spectrum In the figure the angle dependence for SS433 spectrum is shown. ...
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Ссылки http://www.iki.rssi.ru/galeev/astro2007/krivosheyev2007.pdf -- 389.1 Кб -- 27.02.2008
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8. Fundamentals of Mechanics
.
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Ссылки http://zebu.uoregon.edu/1999/ph161/l4.html -- 4.3 Кб -- 21.01.1999
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9. CSPICE Routines: SCTIKS_C
... Abstract Convert a spacecraft clock format string to number of "ticks". ... Detailed_Input sc is the NAIF ID number for the spacecraft whose clock string is being converted. clkstr is a character string representing a spacecraft clock time, WITHOUT PARTITION NUMBER. ... scencd_c converts a clock string to the number of ticks it represents since the beginning of the mission, and so uses partition information. sctiks_c just converts to absolute ticks. ... The SCLK string includes a partition number. ...
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Ссылки http://www.stsci.edu/~sontag/spicedocs/cspice/sctiks_c.html -- 12.2 Кб -- 17.12.2005
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10. Fit a source with a small number of net counts
Next: Inspection of results Up: *fit* - Fit Data Previous: Verbose Mode . If the number of net counts for a source is less than it is impractical to fit the data in all 34 energy bits. However, if the flux is required, then a fit must be performed first. ... Fit will then calculate the normalization of the model and xflux can be used to determine the flux and luminosity of the source from the best fit model. xs> fit rebin=yes . ...
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Ссылки http://hea-www.harvard.edu/PROS/PUG/node153.html -- 3.9 Кб -- 01.10.2012
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11. http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0112-1-0.ps.gz
XMMNewton CCF Release Note XMMCCFRELnonumberassigned EPIC Spectral Response Distribution R. D. Saxton 27 Feb 2002 1 CCF components Name of CCF VALDATE CAL VERSION XSCS flag EMOS1 QUANTUMEF 0010.CCF 20000101 NO EMOS2 QUANTUMEF 0010.CCF 20000101 NO EPN QUANTUMEF 0010.CCF 20000101 NO 2 Changes Four new extensions, FRACTION CHANNEL, FRACTION ENERGY, QE TOTAL and EBINS FRACTION have been added. ... EBINS FRACTION ENERGY: The energies used to define the QE TOTAL array. ...
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Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0112-1-0.ps.gz -- 55.4 Кб -- 01.03.2002
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12. Number Theory Semester - Poncelet Laboratory
January - June 2010 . ... Number theory seminar . ... There is a weekly number theory seminar taking place on Thursdays at the Independent Universty of Moscow (11, Bolshoi Vlassievsky pereulok), room 308. ... Thursday 20 May 2010 . 18:00-19:30 . ... p-adic representations of Gal(\bar{Q_p}/Q_p) III . ... p-adic representations of Gal(\bar{Q_p}/Q_p) II . ... S. Rybakov (Poncelet Laboratory) . Representations of Gal(\bar{Q_p}/Q_p) in GL_n(\bar{F_p}) . ... Thursday 1 April 2010 2010 . ...
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Ссылки http://www.mccme.ru/lifr/zykin/eng/seminar.html -- 9.8 Кб -- 30.06.2010
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13. Spectral-Line Observing
... We will consider the rms, (K), for observations with a receiver of system temperature, T , frequency resolution, per polarization, and total integration time per observing cycle, . ... For ``in-band'' frequency switching, the line under investigation is always in the observing band. ... Position Switching or ``Out-of-Band'' Frequency Switching: Here the line is only observed for one half of the time, with noise being present all of the time. ...
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Ссылки http://www.naic.edu/~astro/guide/node15.html -- 10.0 Кб -- 22.02.2012
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14. DRAO surveys
... Higgs, 1989; DRAO 1991. ... 12-13 RA (hours) 15-16 RA (min) 18-22 RA (sec) (XX.XX) 24-28 RA error (sec) (XX.XX) ( blank = unknown ) 30 Sign of declination 31-32 DEC (degrees) 34-35 DEC (arcmin) 37-40 DEC (arcsec) (XX.X) 42-45 DEC error (arcsec) (XX.X) ( blank = unknown ) 47 Epoch of coordinates (1=B1950, 2=J2000, 3= unknown ) 49 Type of position determination (1=rough estimate, 2=centroid, 3=peak, 4=fitted Gaussian, 5= unknown ) 51-56 Flux #1 ( variable format ) 58-62 Error in ...
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Ссылки http://www.sao.ru/cats/doc/DRAO.html -- 4.7 Кб -- 18.03.2015
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15. The format of STARTABLE
... Inside IDL, STARTABLE is in the table format. ... STAR (string) Identifier of form CCCNNNNNN/CCCNNNN . ... RA (double) Right Ascension [h] . ... BAT (short int) Number in Batten's Catalogue . ... BSC (short int) Number in Bright Star Catalogue . ... ADS (short int) Number in Aitken Double Star Catalogue . ... WDS (long int) Number in Washington Double star catalog . MV (float) Johnson V magnitude (for combined system if multiple) . ... TYPE1 (float) Floating point spectral type of component 1 . ...
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Ссылки http://www.eso.org/~chummel/oyster/manual/node100.html -- 8.5 Кб -- 28.04.2015
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16. Naughty Number Nine
... Number nine will put you on the spot. ... Naughty number nine. ... Is that it's one less than ten. You see, nine is the same as ten minus one. ... I mean, eight times nine is 80 minus eight, . And seven times nine is 70 minus seven, . And six times nine is 60 minus six. ... With naughty number nine. ... One times nine is nine, and two times nine is 18. Mean ol' number nine. ... Eight times nine is 72, and nine times nine is 81, . ... With naughty, nasty, mean ol' number nine. ...
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Ссылки http://crydee.sai.msu.ru/ftproot/pub/rec/music/lyrics/cs-uwp/s/schoolhouse.rock/9.html -- 3.5 Кб -- 09.04.1995
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17. http://www.wdcb.ru/stp/data/sudden.com/STORM1_1868-1967/storm1_fmt.txt
... Column Fmt Description ---------------------------------------------------------------------- 1 A1 Blank 2- 5 I4 Year (19__) 6- 8 A3 Blank 9-10 I2 Month 11-13 A3 Blank 14-15 I2 Day 16-17 A2 Blank 18-20 F3.1 Time in tenths of hour 21-24 A4 Blank 25 I1 Code number of the ssc in the N collection (0, 1, 2 or 3 -- the number 9 occurs when no record was available) 26-29 A4 Blank 30 I1 Code number of the ssc in the T ... 181-182 A2 Blank 183-185 I3 Order number of ssc in the year. ...
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Ссылки http://www.wdcb.ru/stp/data/sudden.com/STORM1_1868-1967/storm1_fmt.txt -- 9.3 Кб -- 18.09.2015
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18. How Do You Feel About Numbers? - an Astronomy Net Exploration Forum Message
Astronomy Discussion Forums . Forums: . ... How Do You Feel About Numbers? ... Post Message | ... Posted by Richard D. Stafford, Ph.D. on September 15, 2002 16:22:25 UTC . ... Wait - harvey1 - September 15, 2002 - 22:20 UTC . I don't follow you! - doctordick - September 16, 2002 - 14:59 UTC . ... www.astronomy.net . About Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...
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Ссылки http://www.astronomy.net/forums/exploration/messages/14.shtml -- 18.0 Кб -- 09.04.2016
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19. Increasing number of files in system
... Forum: The Linux Kernel Hackers' Guide . ... Keywords: kernel tuning, file handles, Bus error . ... Increasing number of open file handles in kernel. I have successfully increased the number of files on my system (Linux 2.0.30) by editing the following file: . ... I also increased NR_INODE to 5000, and NR_FILE to 4096. I then rebuilt the Kernel (and modules for good measure) and installed the new image. ... Increasing number of open files parameter by Simon Cooper . ...
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Ссылки http://www.arcetri.astro.it/irlab/doc/library/linux/khg/HyperNews/get/khg/59/2.html -- 3.5 Кб -- 23.03.2000
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20. Титарчук Лев Григорьевич (NRL)
... We show the analysis of low-hard and intermediate states of sources XTE J1550-564, H 1743-322, GX 339-4, XTE J1859-226, XTE J1650-500 and GRS 1915+105. ... Directly applying the scaling technique we also obtain that a ratio of the BH masses in XTE J1859-226 and in XTE J1550-564 is , and the corresponding ratio for XTE J1650-500 and XTE J1550-564 is . These values of scaling factors r implies that BH masses are ; solar masses in XTE J1859-226 and XTE J1650-500 respectively. ...
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Ссылки http://hea.iki.rssi.ru/conf/hea2007/abstracts/node70.html -- 6.1 Кб -- 19.12.2007
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