| : 342959 (213 ) ---- : 0.83. |
41. http://www.pereplet.ru/nauka/Soros/pdf/9902_091.pdf
... . . , ,, ,̜ , . .. , " " ,,, .., 1999 , , - , . ... XX , .. 91 , , , . ... 1 -0,4 3 0 0,4 (B-V)0 0,8 1,2 1,6 -2 5 0 7 V 9 2 Mv 4 11 6 M45 13 8 0 0,4 0,8 B-V 1,2 1,6 . ... .. 93 1950 +24 +22 +20 +18 +16 +14 +12 Ori Ori Ori +6 50 40 30 20 10 0 1950 Tau +10 +8 20 10 0 6 h 5h 50 40 30 20 10 0 4h 50 40 +4 3h . ...
42. Galaxy
... : 10 2016 . 206- , Galaxy Evolution Explorer, - . 24 2004 . GJ 3685A. ( GJ 3685A ) . ...
43. Keywords_94
... PREBIOLOGICAL PANSPERMIA AND THE HYPOTHESIS OF THE SELF-CONSISTENT GALAXY ORIGIN OF LIFE . ... The evolution of the civilization is even faster. ... Thus the scale of the duration of the 'natural' planetary prebiological chemical evolution may be ~10 billion years (and there is no time for such long prebiological evolution on the Earth of course). ... In this situation the prebiological chemical evolution may not be isolated on any single planet from the all-Galaxy prebiological infection. ...
44. STellar EVolution (STEV)
. . . STEV . . STEV . . . . . . . . . . .
45. Telescope.ru -
. ... . ... 0 0 . ... Celestron . ... . ... 49 990 . ... . ... , , , , . ... Copyright TELESCOPE.RU, 2016. ...
46. astro-ph
... arXiv.org . astro-ph . ... We fit the near-infrared to radio spectral energy distributions of 30 luminous and ultra-luminous infrared galaxies with pure starburst models or models that include both starburst and AGN components to determine important physical parameters for this population of objects. In particular we constrain the optical depth towards the luminosity source, the star formation rate, the star formation efficiency and the AGN fraction. ...
47. Galaxies And How To Observe Them+ - -
> > . Galaxies And How To Observe Them+ - . ... . ... R.Bak . ... , - - , . ... A= . ... ( ) .. ( ) .. ( ) .. ...
48. Black-hole Galaxy Model Of Dark Matter - an Astronomy Net Blackholes2 Forum
Blackholes2 Forum Message . Forums: . Atm Astrophotography Blackholes Blackholes2 CCD Celestron Domes Education . ... Discussion Forums | ... Black-hole Galaxy Model Of Dark Matter . ... included the following paper on a Black-hole Galaxy model of Dark Matter. ... 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" . ...
49. Les galaxies barres sont moribondes | Ciel et Espace
... Ciel Espace, le magazine qui vous guide toujours plus loin . ... des actualits . ... les plus belles images de l'Univers dcryptes pour vous . ... des pages consacres la publication de vos photos Mais c'est aussi une vraie communaut avec laquelle partager votre passion et nourrir votre curiosit. Accueil Les galaxies barres sont moribondes . ... Les galaxies spirales dont une barre d'toiles traverse le centre (dites barres) sont plus vieillissantes que celles dnues de barre. ...
50. http://sn.sai.msu.ru/~sil/preprints/postbr2.pdf
... All the galaxies are divided into 4 groups depending on the environment type; every subsample contains more than 10 galaxies. ... An effect of environments is seen both for the nuclei and for the bulges: if we consider the clusters (Virgo and Ursa Ma jor) and group centers as dense environments and the field and group periphery as sparse environments, then in the dense environments the stellar populations of S0s are in average older by 45 Gyr than in the sparse ones. ...
51. Anatoly V. Zasov
... Field of research: Extragalactic astronomy. ... NASA Astrophysics Data System (ADS) Abstract Service . ... CADC Home Page . ... CCD Images of Galaxies . ... RUSSIAN LINKS . ... UA Astronomy Personal Home Page - Bill Keel . ... The Shape of the Rotation Curves of Edge-on Galaxies, by A.V.Zasov and A.V.Khoperskov, 2003. ... A Thickness of Stellar Discs, by A.V.Zasov, and D.V.Bizyaev, 2003 . Minimum Velocity Dispersion in Stable Stellar Disks, by A.V.Khoperskov, A.V.Zasov, and N.V.Tyurina, 2003 . ...
52.
. Mosenkov A.V., Sotnikova N.Ya., Reshetnikov V.P. 2MASS photometry of edge-on spiral galaxies - I. Sample and general results, 2010, MNRAS, V.401, pp.559-576 . Sotnikova N.Ya., Reshetnikov V.P., Mosenkov A.V. Bulges and discs of spiral galaxies: edge-on perspective, 2010, submitted to Astron. Astrophys. Trans., talk presented at the meeting "Dynamics and Evolution of Disc Galaxies" held in Moscow and Pushchino, Russia, May 31 - June 4th, 2010.
53. http://www.iki.rssi.ru/comp/2012/gilfanov.htm
. ... . ... , L X / SFR - 2 z 2. ...
54. http://www.astro.louisville.edu/shared_skies/archive/select/unusual/hoags_object/20130412/hoags_object_wikipedia_20130422.pdf
... Courtesy of NASA/ESA Observation data (J2000 epoch) Constellation Right ascension Declination Redshift Distance Type Serpens Caput 15h 17m 14.4s[] +21 35 08[] 12,74050 km/s[][1] 60030 Mly (1838 Mpc)[1] SA0(r) [citation needed ] [a] Apparent dimensions (V) 0.28 0.28[] Apparent magnitude (V) 16.0[] Notable features Ring galaxy Other designations PGC 54559,[] PRC D-51[] See also: Galaxy, List of galaxies Hoag's Object is a non-typical galaxy of the type known as a ring galaxy. ...
55.
... . ... , , 130 . ... . Galaxy Evolution Explorer (GALEX) 83. , , 15 . . ... . ...
56. Arkhipova Natalya Anatolievna, Astro Space Center (ASC)
... 2001 - present-day Researcher in Theoretical Department of Astro Space Center of Lebedev Physical Institute ot RAS . ... Department Number . ... Astro Space Center . ... arna@lukash.asc.rssi.ru . ... Arkhipova N.A., Komberg B.V., Lukash V.N., Mikheeva E.V., "Population of Cosmic Voids", Astronomy Reports 51, pp 787-796 (2007) . ... Surdin, V.G., Arkhipova, N.A., "Influence of dissipation and dynamical friction on the number of globular clusters in a galaxy", Astronomy Letters, Vol.24, p.343 (1998) ...
57. MILLIMETRON
... The project assumes creation of an international space observatory - the interferometer "Earth - Space - Space" in order to perform of astronomical investigations in millimeter, submillimeter and infrared regions with extremely high sensitivity (to a few nanoJanskies units of flux density in continuum spectrum) and extremely high angular resolution (to a parts of microsecond of arc or, possibly, nanosecond). ... radio-interferometric channels of the system "Space - Space", region 0.2 - 3 mm; . ...
58. N6, 1996
... Telephone: 81 3 5620 9429 International Travel Division Facsimile: 81 3 5620 9400 Convention Center (CD100993-543) 5-5-2, Kiba, Koto-ku, Tokyo135, Japan SCIENTIFIC PROGRAMME: OVERVIEW Invited Discourses JD 1 The Hubble Deep Field R.E.Williams JG 2 The Cataclysmic Variable Stars B.Warner JD 3 Black Holes in the Universe I.D.Novikov Symposia S 183 Cosmological Parameters and the Evolution pf the Universe S ... The dates for this workshop are 3 - 5 March, 1997. ... March 3-5, 1997: Workshop. ...
59. arxiv:1012.0765 ,
... ? arxiv:1012.0765 , . ... arxiv:1012.0765 , 2010 (Understanding exoplanet formation, structure and evolution in 2010) . ... : 07.12.2010 [10:46:05] arxiv:1012.0765 , 2010 (Understanding exoplanet formation, structure and evolution in 2010) . ...
60. XMM Deep Survey Simulations
... QSO spectra in the ROSAT band are steeper than the background at harder energies, and furthermore at fluxes below 1E-14 ergs/(s cm) the quasar source counts flatten off and are replaced by more numerous populations of relatively low red-shift objects, apparently Narrow Emission Line Galaxies (NELG). ... We extracted the luminosity function from ROSAT Deep Survey results, and extrapolated by a factor of 2 - 3 to account for changes expected in the harder XMM band. ...