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1. http://astro.uni-altai.ru/AFgalleries.html
[ Сохраненная копия ]  Ссылки http://astro.uni-altai.ru/AFgalleries.html -- 1.1 Кб -- 01.10.2012
[ Сохраненная копия ]  Ссылки http://astroclub.ru/ -- 1.2 Кб -- 09.04.2016
[ Сохраненная копия ]  Ссылки http://astronomy.tomsk.ru/google.php -- 1.3 Кб -- 01.10.2012
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2. Astronomy HyperText Book: Fusion Sequences in Stars
All stars derive their energy through the thermonuclear fusion of light elements in to heavy elements. High temperatures are required so that the mutual electrostatic repulsion of the protons in each fusing atomic nucleus is overcome. ... Elements with more protons in their nuclei require higher temperatures. ... This sequence is now shown in the animation below. ... First Step of the Proton-Proton Chain Narration . Second Step of the Proton-Proton Chain Narration . ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/textbook/energygen.html -- 3.0 Кб -- 14.02.1995
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3. The Sun Energy Source Is Not Nuclear Fusion But Magnetic Fields. - an Astronomy
Bigbang Forum Message . Forums: . ... The Sun Energy Source Is Not Nuclear Fusion But Magnetic Fields. ... The sun is not heated by fusion reaction but by magnetic fields coming from the galactic center. The nuclear fusion is a by product of the magnetic fields heating. ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.net/forums/bigbang/messages/882.shtml -- 14.2 Кб -- 09.04.2016
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4. High Energy Astrophysics Today and Tomorrow
... А.М. Белобородов (Колумбийский университет, США) . ... Рабочий язык конференции - русский. ... Е.М.Чуразов, д.ф .- м.н . А.А. Вихлинин, проф. д.ф .- м.н . М.Р.Гильфанов, д.ф .- м.н . М.Н.Павлинский, д.ф .- м.н . М.Г.Ревнивцев, д.ф .- м.н . С.Ю.Сазонов. д.ф .- м.н . М.Н.Павлинский (председатель), к.ф .- м.н . А.В.Мещеряков (зам. председателя), Н.Л.Александрович, к.ф .- м.н . В.А.Арефьев, к.ф .- м.н . Р.А.Буренин, П.Болдин, Н.П.Васильева, к.ф .- м.н . А.А.Воеводкин, В.Воробьев, А.Е.Елкин, ...
[ Сохраненная копия ]  Ссылки http://hea.iki.rssi.ru/conf/hea2012/ -- 19.4 Кб -- 27.02.2014
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5. Russian High Energy Neutron Detector for 2001 MARS ODYSSEY
. H . E . N . D . IGH . NERGY . EUTRON . ETECTOR . Copyright © 2000-2008, Russia, Space Research Institute
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/hend/ -- 5.3 Кб -- 07.03.2012
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/hend/ -- 5.3 Кб -- 07.03.2012
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6. Energy
... Belts . ... Speed of motion is " kinetic energy ", like the energy of a turning flywheel or of the wind hitting a windmill, both of which can move machinery. ... As the hot gas of the corona--a plasma, really--expands upwards, its heat is converted to the kinetic energy of a fast flow, streaming outwards: the solar wind . Four or five days after leaving the Sun, solar wind plasma hits the magnetosphere, an obstacle in its path. ... How is solar wind energy transmitted to the magnetosphere? ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/mirrors/stern/Education/wenergy.html -- 8.9 Кб -- 21.12.2007
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7. High Energy Andromeda
... 7.01.2016 . ... Credit Copyright: NASA , JPL-Caltech, GSFC, NuSTAR , GALEX , Explanation: A mere 2.5 million light-years away, the Andromeda Galaxy, also known as M31, really is just next door as large galaxies go. ... Andromeda is close enough that NuSTAR can examine its population of X-ray binaries in detail, comparing them to our own. ... January 2016 . ... 2015 2016 . ... Publications with keywords: M 31 - Andromeda galaxy - X-ray . Publications with words: M 31 - Andromeda galaxy - X-ray . ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/msg/1353061 -- 14.6 Кб -- 07.01.2016
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8. APOD: 2016 January 7 - High Energy Andromeda
... 2016 January 7 . High Energy Andromeda . Image Credit: NASA , JPL-Caltech, GSFC, NuSTAR , GALEX , . ... In this (inset) scan, image data from NASA's Nuclear Spectrosopic Telescope Array has yielded the best high-energy X-ray view yet of our large neighboring spiral, revealing some 40 extreme sources of X-rays , X-ray binary star systems that contain a black hole or neutron star orbiting a more normal stellar companion. ... About APOD | ... NASA Official: Phillip Newman Specific rights apply . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap160107.html -- 4.9 Кб -- 10.04.2016
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9. High Energy Astrophysics
... CfA Home . HCO Home . SAO Home . ... Welcome to CfA . CfA History . ... Laboratory Astrophysics . Extreme Astrophysics . ... 617) 495-7210 . ... 617) 495-7044 . ... 617) 495-7265 . ... HEA Research . ... HEA Home Page . CFA/HEA Home Page . ... High Energy Astrophysics Division (HEAD) . Chandra X-ray Center . ... Chandra Cluster Cosmology Project . Chandra Multiwavelength Project (ChaMP) . ... Chandra-Planck Clusters Project . ... CfA Virtual Observatory Project . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/ -- 33.5 Кб -- 09.04.2016
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10. http://www.arcetri.astro.it/science/chianti/chianti_3.03/elements/fe/fe_24.html
energy levels (1-24): Sugar, J., and Corliss, C., 1979, J. Phys. Chem. ... Data, 8, 865. %energy levels (1-24): Kelly, R. L., 1987, J. Phys. Chem. ... Data 16, Suppl. 1. %comments: 5s from Kelly % Theoretical energy levels (1-24): Zhang,H.L., Sampson,D.H., Fontes,C.J., 1990, Atomic Data and Nuclear Data Tables, 44, 31. Innershell energy levels: NIST database %Innershell theoretical energy levels: Goett, S.J., Sampson, D.H., 1983, ADNDT, 29, 535 % % E. Landi - July 1999 . ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/chianti/chianti_3.03/elements/fe/fe_24.html -- 2.8 Кб -- 20.07.2000
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11. A New Database of Observed Spectral Energy Distributions of Nearby Starburst
We present a database of UV-to-FIR data of 83 nearby starburst galaxies. ... The NIR data are from new observations obtained at the NASA/IRTF and the Mount Laguna Observatory, combined with the published results from observations at the Kitt Peak National Observatory. ... In conjunction with IRAS and ISO FIR flux densities, all these data form a set of observed spectral energy distributions (SEDs) of the nuclear regions of nearby starburst galaxies. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2002ApJS..143..377W.html -- 4.8 Кб -- 21.01.2016
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12. Encircled energy correction
... arfgen (arfgen-1.75.6) [?? ... In the case of a point source, arfgen can correct for the flux that is outside the region(s) over which the spectrum was accumulated. ... The correction works by taking a model of the PSF from the CAL, centred at the source position and calculating the total fraction of that PSF within the regions of interest. To enable the encircled energy correction for point sources, the parameter extendedsource must be set to false , as well as modelee being set to true . ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/arfgen/node27.html -- 5.6 Кб -- 22.10.2008
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13. Energy distribution
... One of the most widely used tools of Fourier analysis is the Parseval theorem. It enables the experimentalist to view how the `energy' in the signal is distributed among frequencies. The Fast Fourier Transform (FFT) algorithms have made power spectra one of the obvious diagnostics tools during data acquisition, and energy maps are a versatile alternative. ... The result is an energy map (Fig. 9), showing the distribution of energy corresponding to the wavelet map (Fig. ...
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/~vab/Wavelet.rsc/Tutor.dir/node7.html -- 3.5 Кб -- 12.04.1998
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14. KINETIC ENERGY
. First page Back Continue Last page Graphics .
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/slides/nh2/text13.html -- 1.6 Кб -- 05.07.2002
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15. WKB and eikonal approximations (high energy - HEA)
The approaches mentioned in the section title belong to one family which is called in Newton's book [ 56 ] the short waves or high energy approximation (HEA). It means the scattering by soft particles (or potentials) in the case of the wavelengths short in comparison with the particle size (or correspondingly the case of scattering of high energy particles by the potentials). ...
[ Сохраненная копия ]  Ссылки http://www.astro.spbu.ru/DOP/3-REVS/KHLEB1/node16.html -- 7.1 Кб -- 19.11.2010
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16. ESO - Thesis Topic: Cepheid stars, Ho and Dark Energy: precision stellar
... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: Cepheid stars, Ho and Dark Energy: precision stellar astrophysics for precision cosmology . ... Observing with ESO Telescopes . ... ESO-MIDAS . ... ESO Data . ... ESO HST Image Galleries . ... ESO Data Access Policy . ... ESO Science Newsletter . ... ESO Annual Reports . ... Seminars at ESO Santiago . ... Seminars at ESO Garching . ... ESO Telescope Bibliography . ... Last Update: 03.02.16 ESO . ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/sci/activities/thesis-topics/abstr-romaniello01.html -- 28.5 Кб -- 10.04.2016
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17. Dark matter and dark energy: the deepest mysteries in astronomy | Astronotes
Astronotes Armagh Planetarium's Stellar Blog! ... Our Galaxy . ... Space Flight . ... Here be dark matter! ... This is dark energy, a force which permeates all space. ... No one knows what dark energy and dark matter are; researchers study the light of far off galaxies to see how these elusive quantities effect them. ... Dark matter and dark energy are utter mysteries today but so were electricity, magnetism and radioactive decay once. ... Some times ?Dark Matter? is real, remember Neptune! ...
[ Сохраненная копия ]  Ссылки http://www.armaghplanet.com/blog/dark-matter-and-dark-energy-the-deepest-mysteries-in-astronomy.html -- 44.7 Кб -- 09.04.2016
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18. Optical and other high energy emission
Next: The interstellar medium Up: An overview Previous: Radio pulse characteristics . Mostly the very youngest pulsars . Just 3 pulsars detected at Optical Wavelengths . Crab, Vela, B0540-69 . X-ray - 27 detected, 13 pulsed . Gamma ray - 6 detected all pulsed . Radio emission of spin down energy . ... Need radio ephemeris . 18000 pulse periods elapse between each EGRET photon detected from the Crab pulsar . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/research/pulsar/Tutorial/tut/node13.html -- 4.0 Кб -- 04.02.2013
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19. Spectral energy distribution
... In brief: the frequency-dependent radiative transfer equation is solved for a dust under assumption of spherically-symmetric geometry for its distribution taking into account particle size distribution and quantum heating effects for the very small dust particles. ... Table: Model parameters for IRAS04296+3429. ... parameter . ... hot dust shell) . ... The best fit to the spectral energy distribution of IRAS04296 is shown by heavy solid line (see Table2 for details concerning parameters of the model...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/ssl/IRAS04296/node8.html -- 17.5 Кб -- 02.10.2012
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/ssl/IRAS04296/node8.html -- 17.5 Кб -- 01.10.2012
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/ssl/IRAS04296/node8.html -- 17.5 Кб -- 01.10.2012
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20. Planckian Energy
About maximal luminosity in the Nature and stability black holes under planckian mass, "Concluding remarks", Vulcano workshop 1992, Conference Proceedings, vol.40, p.499, Italian Physical Society(Eds. F.Giovannelli and G.Mannocchi), Bologna, 1993. "Planckator: an Astrophysical Accelerator to Planck Energies", The talk on American Physical Society Meeting,Bull.Amer.Phys.Soc. 41,No.2, 927, 1996 . Planckator Back .
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~lipunov/planck.html -- 1.8 Кб -- 16.06.2000
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