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1. Late Stages of Stellar Evolution
... Australia Telescope Steering Committee . ... Parkes radio telescope . ... Late Stages of Stellar Evolution . Welcome to the home page of the Late Stages of Stellar Evolution" We are a research group which operates within the Astrophysics Group of the Australia Telescope National Facility. ... To investigate the late stages of stellar evolution and in particular the role of stellar mass-loss in the evolution of asymptotic giant branch stars, proto-planetary nebulae and extremely massive stars. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/plintel/groups/lsse/LsseHomePage.html -- 52.2 Кб -- 28.02.2014
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2. Astrophysics Group Galaxy Formation and Evolution
... Astrophysics Group . ... Galaxy Formation and Evolution . ... Gas heating and outflows driven by accreting supermassive black holes (quasar phase) may affect the evolution of star formation in their host galaxy. ... The starburst galaxy M82, which expels dust and metal enriched gas out of its disk . ... The interstellar medium (ISM) plays a central role in galaxy evolution, providing the fuel for star formation and also hosting the ?fossil record? of the galaxy formation history. ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/research/extragalactic-group-2/ -- 17.0 Кб -- 10.04.2016
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5. Parameters of binary compact star evolution
... Figure: Massive binary evolutionary track. ... A short glance to this track is sufficient to understand that there are a lot of evolutionary scenario parameters, which affect different stages of the binary evolution. Fortunately, a very limited number of parameters has effect on the compact binary merging rate. ... The most important (and practically unique) parameter changing the galactic binary NS merging rate is the distribution of an additional (kick) velocity imparted to NS at birth. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~lipunov/kionewht/node9.html -- 7.2 Кб -- 16.06.2000
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6. The Evolution of Galaxies through the Neutral Hydrogen Window The Evolution of
. The proceedings of the conference The Evolution of Galaxies through the Neutral Hydrogen Window have now been published. The proceedings can be accessed online at the AIP website. Conference attendees have access for 1 year as part of their registration, using the username and password provided by the conference organisers. If you have not received this, or have lost it, please contact rminchin (at) naic.edu. Last updated: Friday, 11-Apr-2014 16:52:00 AST . E. Momjian R. Minchin
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~astro/hiconference/proceedings.shtml -- 3.0 Кб -- 10.04.2016
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7. Informational system "Evolution of RG"
The project of the informational system creation on the problem of evolution of radio galaxies, as a part of the "Big Trio" project aimed on studing of distant radio galaxies, is designed. This system allows a user to operate with simulated curves of spectral energy distributions (SED) to estimate ages and redshifts by photometry data. Authors use SEDs of several models for different types of galaxies. ... The HTTP and e-mail access is organized to this system. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/sed/ -- 4.7 Кб -- 15.07.2001
[ Сохраненная копия ]  Ссылки http://sed.sao.ru/ -- 4.7 Кб -- 15.07.2001
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8. ESO - Thesis Topic: ALMACAL: the evolution of the molecular gas in galaxies
... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: ALMACAL: the evolution of the molecular gas in galaxies using ALMA calibrator observations . ... ALMA . ... ESO-MIDAS . ... It is therefore essential to probe the evolution of cold gas over cosmic time. ... We are looking for an enthusiastic PhD student who is interested in working with us in using ALMACAL to address exciting and topical science questions related to the evolution of molecular gas in galaxies. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/sci/activities/thesis-topics/abstr-zwaan1.html -- 29.5 Кб -- 10.04.2016
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9. Web-Site Content and Internet Access
Next: Measuring Internet Access Up: Widening Access Previous: First Observation of a Contents . ... The Observatory web-site also increasingly makes available the results of astronomical observations carried out at Armagh, for example images of meteorological or space-weather events such as aurorae (see http://star.arm.ac.uk/images/aurora-2003-Oct/), and transient astronomical events such as occultations, eclipses and transits. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/annrep/annrep2004/node66.html -- 4.1 Кб -- 19.04.2005
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10. ASP: Family ASTRO: History and Evolution
Family ASTRO was initially developed to expand the ASP?s flagship program Project ASTRO?, which has partnered thousands of volunteer amateur and professional astronomers around the country with classroom teachers and students in their communities. ... Since then, we?ve trained not only many Project ASTRO partners, but also hundreds of other educators across the country to use our series of Leader Kits and Take-Home Activities to lead fun, hands-on Astronomy Events in their communities. ...
[ Сохраненная копия ]  Ссылки http://www.astrosociety.org/edu/family/about/history.html -- 9.1 Кб -- 02.10.2012
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11. Galaxy formation and evolution in cosmic voids
Galaxy formation and evolution in cosmic voids . ... Pustilnik S.A. (SAO RAS) - head. ... Perepelitsyna Y.A., Pustilnik S.A., Kniazev A.Y., "Study the evolution of galaxies in the near void Lynx-Cancer", abstracts in Russian conference "Galaxies", Essentuki, 24-27.11.2014 . ... Safonova E.S., Pustilnik S.A., Kniazev A.Y., "The study of the evolution of galaxies in the Eridanus Void", abstracts in Russian conference "Galaxies", Essentuki, 24-27.11.2014 . 19 December 2014 ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Laboratory/Current/GFEV_eng.html -- 6.4 Кб -- 29.12.2014
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12. COALA - Computational Astrophysics Laboratory
Amanda Karakas One of the most important research fields in astrophysics is the study of the origin of the elements. ... Asymptotic Giant Blanch (AGB) Stars: For low and intermediate-mass stars (with initial masses between about 0.8 to 8 solar masses) the most important nucleosynthesis occurs when stars evolve off the main sequence to the giant branches. ... This indicates that these stars obtained their unusual abundances via mass transfer from a previous red giant star, that has long evolved away. ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/coala/star.html -- 6.0 Кб -- 01.10.2012
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13. Examples of displaying access permissions
To display the permissions on a single file: ls -l file1 -rw-r--r-- 2 unixjohn doc 3287 Apr 8 12:10 file1 . ... To display the permissions on the contents of a directory: ls -l prototype . ... To display the permissions on each file and directory in your current directory : ls -l -rw------- 1 erpl08 iss 4307 Jun 17 10:00 FAQ.xdh drwx------ 2 erpl08 iss 1024 Jun 17 10:00 SCCS -rw------- 1 erpl08 iss 15119 Jun 17 10:00 commands.xdh -rw------- 1 erpl08 iss 266 Jun 17 10:00 concepts.xdh . ...
[ Сохраненная копия ]  Ссылки http://comet.sai.msu.ru/UNIXhelp/tasks/next.html -- 3.4 Кб -- 17.01.1997
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14. Cosmic evolution in a computer | Astronomy.com
... Tonight's Sky . ... The Magazine . ... Observing . ... Gravitational wave search provides insights into galaxy evolution and mergers . ... The double star 54 Leonis, spiral galaxy NGC 3198, and emission nebula NGC 3199 . ... Astronomy for Kids . ... Cosmic Adventures . ... Cosmic evolution in a computer . ... V irgo Consortium astrophysicists used a 25-terabyte databank to create a computer simulation showing cosmic structure's evolution. ... Get instant access to subscriber content on Astronomy.com...
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/magazine/2007/03/cosmic-evolution-in-a-computer -- 62.9 Кб -- 10.04.2016
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15. Dust evolution across the CO snowline in a protoplanetary disk
... General information . ... Staff . Research staff . ... Information . ... Historical highlights . Historical research . ... This process is thought to occur in circumstellar disks of gas and dust around young stars on rather short timescales : infrared surveys show that the number of low mass stars with disks drops dramatically for stars older than 10 Myr, suggesting that in order to form large solids before the disk disperses, the growth process has to take place within a few million years. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/en/home-english/204-scientific-news/1098-snow-alma -- 30.1 Кб -- 10.04.2016
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16. Печь конвекционная_Tecnoeka Evolution EKF 423 M Трубная изоляция Изоком 64*9
... Вес 36.4 кг . ... Бренд: Изоком . ... Строительная изоляция . ... Позитивный качественный детский ковер с изображением сюжета из мультсериала 'Маша и Медведь' украсит интерьер детской комнаты и наполнит мир вашего ребенка яркими и живыми красками. ... Небольшой размер и вес позволит без труда перемещать ковер в разные места комнаты и легко производить уборку под ковром. ... Ковер Маша и Медведь" 80*133 см" - яркий красочный ковер, за которым легко ухаживать сделает уютной комнату вашего ребенка. ...
[ Сохраненная копия ]  Ссылки http://astrokuban.info/astroku2431.html -- 19.9 Кб -- 14.02.2016
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17. The Formation and Evolution of LMC Rich Star Clusters: NGC 1818
... LMC Project Outline . NGC 1818 Initial Results . ... The Large Magellanic Cloud (LMC) is uniquely suitable for the study of massive star clusters at all stages of evolution. By combining HST observations of these clusters with N-body models we hope to understand the origin and evolution of rich star clusters in our own Galaxy, in the LMC, and beyond. ... We aim to combine our HST observations with N-body models to understand the formation and evolution of globular clusters. ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node27.html -- 15.4 Кб -- 12.06.2006
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Еще в разделе: (Показать все результаты (>213) - www.stecf.org/ )

18. Linux I/O port programming mini-HOWTO: Example code
... define BASEPORT 0x378 /* lp1 */ int main() { /* Get access to the ports */ if (ioperm(BASEPORT, 3, 1)) {perror("ioperm"); exit(1);} /* Set the data signals (D0-7) of the port to all low (0) */ outb(0, BASEPORT); /* Sleep for a while (100 ms) */ usleep(100000); /* Read from the status port (BASE+1) and display the result */ printf("status: %d\n", inb(BASEPORT + 1)); /* We don't need the ports anymore */ if (ioperm(BASEPORT, 3, 0)) {perror("ioperm"); exit(1);} exit(0); } /* end of example.c */ . ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/sts/linux/doc/io-portprog/IO-Port-Programming-9.html -- 2.7 Кб -- 28.12.2007
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/sts/linux/doc/io-portprog/IO-Port-Programming-9.html -- 2.7 Кб -- 11.09.2010
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/sts/linux/doc/io-portprog/IO-Port-Programming-9.html -- 2.7 Кб -- 02.10.2012
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19. Star Formation History
... A model for the chemical evolution of a disk galaxy is presented. The model reproduces all the basic . ... investigations of the star formation history. ... the galaxyЫand incorporating a delay in the onset of star formation make it possible to model different scenar- . ios for the evolution of a galaxy's luminosity. ... evolution of massive galaxies. ... of reconstructing the star-formation history and galactic luminosity from observations of galaxies at different . ...
[ Сохраненная копия ]  Ссылки http://www.inasan.rssi.ru/~dwiebe/abstracts/sfrazh.html -- 2.9 Кб -- 27.09.2012
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