Astronet Ïîèñê ïî àñòðîíîìè÷åñêèì ñàéòàì English Russian
       
        Òî÷íàÿ ôîðìà ñëîâ   Î ïðîåêòå   Ñàéòû   Ñïðàâêà
Íàéäåíî äîêóìåíòîâ: 273982 (198 ñàéòîâ) ---- Âðåìÿ ïîèñêà: 0.76ñåê.   

1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | Ñëåä.

Ïîêàçàíû äîêóìåíòû, ñîäåðæàùèå ôðàãìåíòû òåêñòà èç äîêóìåíòà
http://www.iki.rssi.ru/comp/2012/gilfanov.htm.

1. http://www.iki.rssi.ru/comp/2012/gilfanov.htm
Ðåíòãåíîâñêîå èçëó÷åíèå ãàëàêòèê â ëîêàëüíîé Âñåëåííîé è íà êîñìîëîãè÷åñêèõ êðàñíûõ ñìåùåíèÿõ. ... Ðàáîòû öèêëà ïîñâÿùåíû èññëåäîâàíèþ ðåíòãåíîâñêîãî èçëó÷åíèÿ îò çâåçäîîáðàçóþùèõ ãàëàêòèê â ëîêàëüíîé Âñåëåííîé è íà êîñìîëîãè÷åñêèõ êðàñíûõ ñìåùåíèÿõ. ... Ñðàâíåíèå ýòèõ äâóõ âåëè÷èí ïîêàçûâàåò , ÷òî óäåëüíàÿ ðåíòãåíîâñêàÿ ñâåòèìîñòü L X / SFR çâåçäîîáðàçóþùèõ ãàëàêòèê íà êîñìîëîãè÷åñêèõ êðàñíûõ ñìåùåíèÿõ íå ìîãëà çàìåòíî ïðåâûøàòü ëîêàëüíîå çíà÷åíèå - íå áîëåå ÷åì â 2 ðàçà íà êðàñíûõ ñìåùåíèÿõ z ˜2. ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.iki.rssi.ru/comp/2012/gilfanov.htm -- 18.9 Êá -- 24.10.2012
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.cosmos.ru/comp/2012/gilfanov.htm -- 18.9 Êá -- 24.10.2012
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>844) - www.cosmos.ru/ )

2. Starburst and Galaxy evolution
Welcome to the Starburst and Galaxy Evolution website.
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.stsci.edu/science/starburst/ -- 1.3 Êá -- 14.12.2001
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>9404) - www.stsci.edu/ )

3. Astronomy HyperText Book: Stellar Evolution
... Stellar Evolution is driven entirely by the never ending battle between Pressure and Gravity . As imbalances are reached, the star is driven to find a new Energy source. ... Pressure and gravitational forces are equal, the star is stable and its core is sufficiently hot to fuse Hydrogen into Helium More about main sequence stars . ... The luminosity generated by the core fusion of Helium into Carbon is far greater than the shell luminosity associated with the fusion of Hydrogen into Helium. ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://zebu.uoregon.edu/textbook/se.html -- 4.8 Êá -- 16.12.1997
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>202) - zebu.uoregon.edu/ )

4. 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. ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.atnf.csiro.au/people/plintel/groups/lsse/LsseHomePage.html -- 52.2 Êá -- 28.02.2014
Ïîõîæèå äîêóìåíòû

5. 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. ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.sao.ru/sed/ -- 4.7 Êá -- 15.07.2001
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://sed.sao.ru/ -- 4.7 Êá -- 15.07.2001
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>58) - sed.sao.ru/ )

6. Evolution of Supernova Explosion Rates in the Universe
Next: The Supernovae Rates Up: No Title Previous: Gravitational wave background from . In this Section we present the results of the Scenario Machine simulation of supernova explosion (SN) rates in the Galaxy for various types of supernovae and apply them for estimating the - dependence for the SN in the Universe (see JÆrgensen et al. 1995[ 80 ]). The Supernovae Rates . Dependence for the Supernova Explosions . for Supernova Explosions . Results and Discussion . ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://xray.sai.msu.ru/~mystery/articles/review/node91.html -- 4.6 Êá -- 29.03.1997
Ïîõîæèå äîêóìåíòû

7. ASP: Cosmology: The Origin, Evolution & Ultimate Fate of the Universe
... Dark Energy (Part of the Hubble Discoveries Series): http://hubblesite.org/hubble_discoveries/dark_energy/ (Flash-based multimedia tutorial on the discovery and meaning of dark energy; includes information on the origin and fate of universe) . ... Cosmology Visualizations from the NASA Universe Forum: http://www.cfa.harvard.edu/seuforum/einstein/resources_visual.htm#featcos (A series of computer visualizations of the evolution and structure of the universe, available in a number of formats.) ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.astrosociety.org/edu/resources/cosmology.html -- 23.8 Êá -- 02.10.2012
Ïîõîæèå äîêóìåíòû

8. ESO - Thesis Topic: Evolution of the interstellar medium in galaxies from
... Science . ... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: Evolution of the interstellar medium in galaxies from redshift 0 to 1.5 . ... Science Users Information . ... Observing with ESO Telescopes . ... Science Software . ... ESO-MIDAS . ... ESO Data . ... ESO Science Newsletter . ... The project is to use public HST NICMOS spectra to search for star formation in galaxies at high redshift and investigate their evolution. ... Return to list of thesis topics ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.eso.org/sci/activities/thesis-topics/abstr-freudling01.html -- 25.7 Êá -- 10.04.2016
Ïîõîæèå äîêóìåíòû

9. Àñòðîíåò > ×àíäðà: îòêðûòèå æåñòêîãî ðåíòãåíîâñêîãî ôîíà
... Àñòðîíåò | ... ïëàíåòà Àñòðîíåò | ... ×àíäðà: îòêðûòèå æåñòêîãî ðåíòãåíîâñêîãî ôîíà . ... Îáñåðâàòîðèÿ ×àíäðà , ÍÀÑÀ . ... Ïóáëèêàöèè ñ êëþ÷åâûìè ñëîâàìè: Chandra - x-ray background - cosmic microwave background radiation - Ðåíòãåíîâñêèé òåëåñêîï - ðåíòãåíîâñêèé ôîí - êîñìè÷åñêàÿ ðåíòãåíîâñêàÿ îáñåðâàòîðèÿ . Ïóáëèêàöèè ñî ñëîâàìè: Chandra - x-ray background - cosmic microwave background radiation - Ðåíòãåíîâñêèé òåëåñêîï - ðåíòãåíîâñêèé ôîí - êîñìè÷åñêàÿ ðåíòãåíîâñêàÿ îáñåðâàòîðèÿ . ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.astronet.ru/db/msg/1162742 -- 24.7 Êá -- 10.11.2006
Ïîõîæèå äîêóìåíòû

10. Astronomy Research Themes : Stellar Evolution
Stars form from interstellar clouds rich in hydrogen....they shine for billions of years, gradually converting hydrogen into helium....when hydrogen is exhausted, they need to find other energy sources....they expand to become giants and supergiants....low-mass stars expel planetary nebulae and become white dwarfs....high-mass stars explode as supernovae, leaving a neutron star or black hole behind. ... What can they tell us about normal stellar evolution ? ... WWW contact: webmaster@star.arm.ac.uk . ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://star.arm.ac.uk/~csj/res-se.html -- 6.0 Êá -- 30.05.2013
Ïîõîæèå äîêóìåíòû

11. The Evolution of Galaxies Seen Through The Neutral Hydrogen Line The Evolution
... Printable versions of this program are available in PDF and plain text . ... Chair: W. Freudling . ... 11:25 HI gas in galaxies from z =0 to z =0.2 PDF . ... Evolution across cosmic time . ... 09:20 Star formation in HI selected galaxies PDF . ... 15:10 Interaction Driven Galaxy Evolution: The Fate of Gas PDF . ... 09:20 HI, H2 and Galaxy Evolution . ... 10:20 Neutral Hydrogen and Star Formation in the Coma Abell 1367 supercluster PDF . ... 14:30 HI and galaxy evolution: what we need to know PDF . ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.naic.edu/~astro/hiconference/draft_sched.shtml -- 17.0 Êá -- 02.10.2012
Ïîõîæèå äîêóìåíòû

13. Galaxy Evolution: The origin and evoltuion of radio sources
... Galaxy Evolution home . Cavendish Astrophysics . ... Cosmological evolution of star-forming galaxies . The origin and evolution of radio sources . ... Radio sources are among the most powerful of the family of Active Galactic Nuclei (AGN). ... The overall properties of radio sources are well predicted by analytical models of self-modifying evolution of the radio source which we have developed, and many of the more unusual structures observed can be reproduced using computational models. ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.mrao.cam.ac.uk/~pa/galaxy_evolution/science_RSorigin.html -- 5.9 Êá -- 24.01.2002
Ïîõîæèå äîêóìåíòû

14. Ïå÷ü êîíâåêöèîííàÿ_Tecnoeka Evolution EKF 423 M Òðóáíàÿ èçîëÿöèÿ Èçîêîì 64*9
... Âåñ 36.4 êã . ... Áðåíä: Èçîêîì . ... Ñòðîèòåëüíàÿ èçîëÿöèÿ . ... Ïîçèòèâíûé êà÷åñòâåííûé äåòñêèé êîâåð ñ èçîáðàæåíèåì ñþæåòà èç ìóëüòñåðèàëà 'Ìàøà è Ìåäâåäü' óêðàñèò èíòåðüåð äåòñêîé êîìíàòû è íàïîëíèò ìèð âàøåãî ðåáåíêà ÿðêèìè è æèâûìè êðàñêàìè. ... Íåáîëüøîé ðàçìåð è âåñ ïîçâîëèò áåç òðóäà ïåðåìåùàòü êîâåð â ðàçíûå ìåñòà êîìíàòû è ëåãêî ïðîèçâîäèòü óáîðêó ïîä êîâðîì. ... Êîâåð Ìàøà è Ìåäâåäü" 80*133 ñì" - ÿðêèé êðàñî÷íûé êîâåð, çà êîòîðûì ëåãêî óõàæèâàòü ñäåëàåò óþòíîé êîìíàòó âàøåãî ðåáåíêà. ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://astrokuban.info/astroku2431.html -- 19.9 Êá -- 14.02.2016
Ïîõîæèå äîêóìåíòû

15. îáçîð "Evolution of astronomical eyepieces" - Òåëåñêîïîñòðîåíèå, îïòèêà
Äîáðî ïîæàëîâàòü, Ãîñòü . ...  òåìå  ðàçäåëå Ïî ôîðóìó . Îáùåðîññèéñêàÿ íåäåëÿ "Àñòðîíîìèÿ íà òðîòóàðå" - 15-17 àïðåëÿ . ... Ïðàêòè÷åñêàÿ àñòðîíîìèÿ ? Òåëåñêîïîñòðîåíèå, îïòèêà (Ìîäåðàòîðû: I.A.R. , Ivan7enych ) ? îáçîð "Evolution of astronomical eyepieces" . ïðåäûäóùàÿ òåìà ñëåäóþùàÿ òåìà . ... 0 Ïîëüçîâàòåëåé è 1 Ãîñòü ïðîñìàòðèâàþò ýòó òåìó. Ãîñòü . ... Åñëè êîìó èíòåðåñíî, èùèòå çäåñü (ïðèäåòñÿ çàðåãèñòðèðîâàòüñÿ íà groups.yahoo.com): . ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.astronomy.ru/forum/index.php/topic,2334.0.html -- 27.9 Êá -- 09.04.2016
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>3614) - www.astronomy.ru/ )

16. Interdisciplinatory Colloquium on cosmic factors of evolution of the biosphere
... A.V. Eliseev . ... V.V. Adushkin, A.V. Vityazev, D.O. Glazachev, G.V. Pechernikova . Exogenous factors in the evolution of the Earth. ... Cosmic rays as a factor of biospheric evolution . ... A.V. Yakushev, N.A. Churilin, V.S. Soina, A.G. Kudinova, E.A. Vorobyova, N.S. Mergelov . ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://comet.sai.msu.ru/~gmr/AC/Colloq2014_e.html -- 3.4 Êá -- 16.10.2015
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>102) - comet.sai.msu.ru/ )

17. Êëþ÷åâîå ñëîâî ?Galaxy Evolution Explorer?
... Àíê à äíÿ . ... Àïïàðàò NASA îáíàðóæèë íåîáû÷íûé õâîñò ó äàâíî èçâåñòíîé çâåçäû . 18-08-2007 17:33 Êîìïüþëåíòà . Êîñìè÷åñêèì àïïàðàòîì NASA Galaxy Evolution Explorer áûëà ñôîòîãðàôèðîâàíà çâåçäà, îáëàäàþùàÿ ÷ðåçâû÷àéíî äëèííûõ õâîñòîì, íàïîäîáèå òåõ, êîòîðûå èìåþò êîìåòû. ... Èñïîëüçóÿ îðáèòàëüíûé òåëåñêîï NASA Galaxy Evolution Explorer, àìåðèêàíñêèå àñòðîíîìû ñìîãëè óâèäåòü, êàê ãèãàíòñêàÿ ÷åðíàÿ äûðà ïîãëîòèëà çâåçäó â ãàëàêòèêå â ñîçâåçäèè Âîëîïàñà. ... Âñå êëþ÷åâûå ñëîâà . ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://astro.uni-altai.ru/events/words/word.html?word=1896 -- 10.2 Êá -- 11.04.2016
Ïîõîæèå äîêóìåíòû

18. SAO: group Physics and Evolution of Galaxies home page
... Laboratory "Structure" was created in 1992 from the temporary scientific group formed in 1988 in SAO RAS. In December 2003 it was transformed into group of Physics and Evolution of Galaxies , which enters into new Laboratory of Extragalactic ASTROPHYSICS and COSMOLOGY. ... Kniazev A.Y. senior researcher, associated foreign member . Kniazeva T.F. junior researcher, associated foreign member . ... Lipovetsky Valentin A. (1945-1996) former leader of the Laboratory . ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.sao.ru/precise/Laboratory/Structure_eng.html -- 3.4 Êá -- 19.12.2014
Ïîõîæèå äîêóìåíòû

19. STellar EVolution (STEV)
. Ãëàâíîå ìåíþ . Ââåäåíèå . Ââåäåíèå â çàäà÷è ïðàêòèêóìà STEV . Îçíàêîìëåíèå . Çíàêîìñòâî ñ óñòðîéñòâîì çàäà÷è STEV . Ðàñ÷åò ìîäåëåé . Ðàñ÷åò ìîäåëåé çâåçä è ýâîëþöèîííûõ òðåêîâ . Çàäàíèÿ . Ó÷åáíûå çàäàíèÿ . Òåîðèÿ . Êðàòêàÿ òåîðèÿ ðàñ÷åòà ýâîëþöèè çâåçä . Íàáëþäåíèÿ . Ñðàâíåíèå òåîðåòè÷åñêèõ ðàñ÷åòîâ ñ íàáëþäåíèÿìè . Ëèòåðàòóðà . Ðåêîìåíäîâàííàÿ ëèòåðàòóðà .
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://observ.pereplet.ru/images/evgeny/stev/stev_web.html -- 3.2 Êá -- 01.10.2012
Ïîõîæèå äîêóìåíòû

20. Galaxy chemical evolution
. Head of the project is A.F.Kholtygin . E-Mails: . afkholtygin <at> gmail.com (A.F.Kholtygin) . yu.mi <at> mail.ru (Yu.V.Milanova) . Please insert @ instead <at> for connection .
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.astro.spbu.ru/staff/afk/GalChemEvol/ProInf.html -- 2.4 Êá -- 19.11.2010
Ïîõîæèå äîêóìåíòû

1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | Ñëåä.


Àñòðîíåò | Íàó÷íàÿ ñåòü | ÃÀÈØ ÌÃÓ | Ïîèñê ïî ÌÃÓ | Î ïðîåêòå | Àâòîðàì

Êîììåíòàðèè, âîïðîñû? Ïèøèòå: info@astronet.ru èëè ñþäà

Rambler's Top100 RFBR ßíäåêñ öèòèðîâàíèÿ