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http://www.stsci.edu/~kgordon/papers/2015A&A...580A..87C.html.

1. Orbits in the period / acceleration plane
... Binary orbits in the acceleration/period plane . Circular Orbits . ... We first present the equations for the period and acceleration of a pulsar in an eccentric binary system as a function of its position in the orbit. ... In Freire, Kramer & Lyne (2001) (from where most of this text and following equations are taken), we describe in more detail how circular binary orbits can be determined from the observed periods and accelerations of the pulsar. ... where is the orbital period of the binary. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~pfreire/orbits/ -- 20.7 Кб -- 20.12.2008
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2. Pictures/Рисунки
. Ranking of stacks by emission of NOx. Two stacks are prevalent, from three to fifteen more are more or less important, and the impact of remainder could be analyzed for possibility of screening them off in order to accelerate calculations. Ранжирование труб по выбросу NOx. Первые две трубы преобладают, трубы от третьей до пятнадцатой более или менее важны, остальные отброшены для ускорения вычислений.
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/ehips/Australia/NCF8.htm -- 1.7 Кб -- 20.09.2001
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3. Calculation of Binary Neutron Star Coalescence Rates
... It is reasonable to expect a priori that the evolution of events is strongly time dependent, so the star formation history in a galaxy is another important parameter. Therefore, by calculating the evolution of events after a -function like star formation burst,   one gets a Green function for any arbitrary star formation history. ... The source evolution in a galaxy with given star formation rate is thus calculated as . ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node97.html -- 8.9 Кб -- 29.03.1997
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4. Important Notes - Please check these
Next: Links to Manual Sections Up: Contents Previous: Contents Contents . ... All VLBA stations have two RDBE units for a total of 8 channels with the DDC. ... SCHED knows how to set up the details for most observations at most stations. ... Please see the discussion of the input parameter PRECDATE . ... Please note that all setup files intended to be used for spectral line observations using DOPPLER must have all channels distinguished, in the setup file, by frequency and polarization. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Tasso.Tzioumis/sched/Important_Notes_Please_chec.html -- 7.3 Кб -- 10.04.2016
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5. Dr. Adam Riess - Dark Energy
... Dark energy is believed to be a component of the Universe whose repulsive gravity is presently accelerating the expansion of the Universe.€а Although it comprises the bulk of the mass-energy of the Universe, its nature is not well understood.€а €аAlbert Einstein originally suggested its existence about 80 years ago. A supernova is the explosive death of a star, which unleashes a burst of light through the cosmos. ... This website is a gift from Nancy Riess . ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/~ariess/darkEnergy_faq.htm -- 11.1 Кб -- 08.01.2008
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6. Own page
. HELLO! HOW ARE YOU? I WONDER! . As you understand, my name is Tanya (KVA - for best friends). My cousin calls me Toussya. My soname is Kondruchenkova. I am seventeen. MY PLANS FOR THE FUTURE .
[ Сохраненная копия ]  Ссылки http://www.schools.keldysh.ru/school1413/eng/the_worl/auth.htm -- 2.4 Кб -- 19.12.2002
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7. Important parts of the kernel
Next: Major services in a Up: Overview of a Linux Previous: Various parts of an . The Linux kernel consists of several important parts: process management, memory management, hardware device drivers, filesystem drivers, network management, and various other bits and pieces. ... Figure 1.1: Some of the more important parts of the Linux kernel. Probably the most important parts of the kernel (nothing else works without them) are memory management and process management. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/sag-0.4/node7.html -- 5.8 Кб -- 04.05.1997
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8. IX International Astronomy Olympiad: Important Notes for interested...
... 2 participants in the younger group. 1 participant in the senior group. prizewinners (I-st or II-nd prize) of the previous IAO not older than the age limit who did not used such a possibility before. 1 team leader (specialist in astronomy or astronomy education). ... For the states, starting their activity in the International Astronomy Olympiad and for the students participating the first time in IAO the age limits for the groups for IAO-2004 are defined as: . ...
[ Сохраненная копия ]  Ссылки http://www.issp.ac.ru/iao/statutes/iao3i04.html -- 7.8 Кб -- 22.03.2006
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9. [sas-uploads] AVISO IMPORTANT - Activar su cuenta
... Previous message: [sas-uploads] AVISO IMPORTANT - Activar su cuenta . Next message: [sas-uploads] sas-1.525.tgz . ... DOCTYPE html PUBLIC -//W3C//DTD XHTML 1.0 Transitional//EN http ://www.w3.org/TR/xhtml1/DTD/xhtml1-transitional.dtd html xmlns= http ://www.w3.org/1999/xhtml head meta http -equiv= Content-Type content= text/ html ; charset=iso-8859-1 / title Untitled Document /title style type= text/css !-- .style3 ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/pipermail/sas-uploads/2010-May/012204.html -- 5.0 Кб -- 07.05.2010
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10. S.P. Korolev RSC Energia - Important Anniversaries of the Corporation
... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Important Anniversaries of the Corporation . 2012 . ... May 15, 2012 - 25 years since the first launch of extra-heavy Energia LV with Pole SC. ... January 12, 2012 - 105 years since the birthday of the Chief Designer of rocket and space technology , the founder of practical cosmonauts, founder and lead of ОКБ-1 (S.P.Korolev RSC Energia), Academician Sergey Pavlovich Korolev . ... 2015 JSC "S.P. Korolev RSC "Energia" . ...
[ Сохраненная копия ]  Ссылки http://www.energia.ru/en/archive/dates_2012.html -- 30.0 Кб -- 09.04.2016
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11. ESO - Why is Technology Transfer important for ESO
European . ... Public . ... ESO for the Public > Doing Business with ESO > Technology Transfer > Importance for ESO . ... Survey Telescopes . ... People and Events . ... Events . ... ESO Press Conferences and Events . ... SO's public relations and educational activities not only increase the awareness of ESO's scientific results among the general public, they are also an important way of stimulating interest in astronomy amongst school children who will be the next generation of European astronomers. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/public/industry/techtrans/Importance.html -- 33.4 Кб -- 10.04.2016
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12. **Important**
. There may be security measures or other authentication procedures in use at your site that prevent you from using the rcp command to copy files from one host to another. Check with your local system administrator to find out what the situation is on your system.
[ Сохраненная копия ]  Ссылки http://comet.sai.msu.ru/UNIXhelp/local/rcp.html -- 1.9 Кб -- 17.01.1997
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13. Marc White - Astrophysicist - The Australian National University
Marc White . ... Turbulent entrainment processes may play an important role in the outflows from young stellar objects at all stages of their evolution. In particular, lateral entrainment of ambient material by high-velocity, well-collimated protostellar jets may be the cause of the multiple emission-line velocity components observed in the microjet-scale outflows driven by classical T Tauri stars. ... University of Amsterdam; STARPLAN, Copenhagen, Jul 2013 . ... E marc.white@anu.edu.au . ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~mwhite/publications.php -- 12.6 Кб -- 09.04.2016
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14. http://zebu.uoregon.edu/~uochep/talks/talks05/G050216-00.pdf
Searching for GRB -GWB coincidence during LIGO science runs Isabel Leonor University of Oregon LIGO-G050216-00-Z Motivation almost 40 years since GRBs were discovered past 15 years has been time of important clues isotropic and inhomogeneous distribution (BATSE); first optical, x-ray, radio counterparts; redshift measurements; association with core-collapse supernovae yet important ...
[ Текст ]  Ссылки http://zebu.uoregon.edu/~uochep/talks/talks05/G050216-00.pdf -- 1848.3 Кб -- 29.03.2005
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15. (Untitled)
... It is precisely these values that are displayed as O – C. In case computed positions of minor planet for all or some part of moments are found without accounting for perturbations, the corresponding moments are followed by asterisk (without perturbations are computed positions for all minor planets if moments of their observations lie outside the basic interval of 16 months or for ordinary ... The coordinate system and type of computed positions are indicated in status bar. ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user3khf.htm -- 2.7 Кб -- 10.04.2016
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16. http://hea-www.harvard.edu/AstroStat/HEAD2013/asiemiginowska_13103_20130408.pdf
Aneta Siem iginows ka 1 Hypothesis Tests Aneta Siemiginowska Harvard-Smithsonian Center for Astrophysics CHASC April 8, 2013 This is one of many statistical topics that was important to Alanna AAS HEAD 2013 Aneta Siem iginows ka 2 Outline · Hypothesis testing: motivation and basic framework · ... See Protassov et al (2002) for details AAS HEAD 2013 Aneta Siem iginows ka Methods: LRT - distribution IMPORTANT! We do not know the true distribution of the test statistics. ...
[ Текст ]  Ссылки http://hea-www.harvard.edu/AstroStat/HEAD2013/asiemiginowska_13103_20130408.pdf -- 746.7 Кб -- 22.04.2013
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17. http://www.izmiran.rssi.ru/~ichertok/SEPs_radio/abstract_en.html
ON THE CORRELATION BETWEEN SPECTRA OF SOLAR MICROWAVE BURSTS . AND SPECTRA OF PROTON FLUXES NEAR EARTH . ... which is equivalent to the power-law index of the integral energy spectrum of protons registered near the Earth orbit in a range of 10-100 MeV , on the one hand, and parameters of microwave bursts such as a ratio of peak fluxes at two frequencies (e.g., 9 and 15 GHz) and a microwave peak frequency f m as well. ...
[ Сохраненная копия ]  Ссылки http://www.izmiran.rssi.ru/~ichertok/SEPs_radio/abstract_en.html -- 13.6 Кб -- 05.05.2009
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18. Important Message
. Here is an applet. It has two parameters -- speed and message. Its alignment is ABSMIDDLE. Here is an applet. It has two parameters -- speed and message. Its alignment is ABSMIDDLE. Here is an another instance of the same applet, but it has a different speed and a different message. Its alignment is RIGHT. Here is an another instance of the same applet, but it has a different speed and a different message. Its alignment is RIGHT. The Java source for the applet.
[ Сохраненная копия ]  Ссылки http://www.sao.ru/cats/~satr/JS/REF/jumping.htm -- 2.9 Кб -- 15.04.1998
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19. Izmccd
Download Izmccd (~2.7 MB). ... a) a choice of the best mode of measurements of stars and objects ("Properties/Measurement"), . b) a choice of reference stars. ... 1) necessity of presence on an image of a plenty of stars (we recommend to apply this mode, if on the frame of reference stars is more 100) . ... Sx and Sy depend from residuals at all reference stars (reference stars are marked by blue color). ... These residuals are the image of the star a minus function of a profile for each pixel. ...
[ Сохраненная копия ]  Ссылки http://www.izmccd.puldb.ru/izmccd4e.htm -- 7.6 Кб -- 17.09.2007
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20. important_en
... 1) A new bright galaxy of the Local Group VV124 (UGC4879) is found. ... Kopylov A.I., Tikhonov N.A., Fabrika S.N., Drozdovsky I.O., Valeev A.F., MNRAS Lett, V. 387, Issue 1, L45, 2008. ... For systems of galaxies in the regions of the Hercules and Leo superclusters the dwarf-to-giant ratio of galaxies in the r-band is evaluated, and it is found that this ratio increases with increasing X-ray luminosity at log L X > 43.5 erg/s. Kopylova F.G., Kopylov A.I., Ast. ... Kopylova F.G., Kopylov A.I., Ast. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/dolly/important_en.html -- 22.4 Кб -- 10.04.2016
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/dolly/important_en.html -- 22.4 Кб -- 09.04.2016
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