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• Константин Александрович Постнов
• Natalya Raguzova Home Page
• Shakura Nikolai Ivanovich

... Planetary Science . Institute . ... ANU Planetary Science Institute, c/o Mount Stromlo Observatory . ... ANU CRICOS # 00120C . ... The ANU Planetary Science Institute (PSI) is a joint venture of the Research School of Astronomy and Astrophysics (RSAA) and the Research School of Earth Sciences (RSES) . In 1995, the first planet orbiting a sun-like star other than our own was discovered. Over 200 extra-solar planets are now known. ...

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• VV29 = Arp 188 = The Chainsaw Galaxy
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• ANU - Research School of Astronomy and Astrophysics - 5th Stromlo Symposium

... We have started a programme of observations of nearby starburst and AGN galaxies with MICHELLE, with the aim of investigating the spatial extent of "Unidentified Infrared Bands (UIB)" emission in these galaxies, and in particular relating these to multi-frequency matched resolution radio maps. ... The spatially integrated MICHELLE spectrum of NGC 7469 in the 8 - 11.5µm range shows an equivalent width of 11.3µm UIB feature which is much smaller then measured by ISO. ...

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Институт Космических Исследований . ... Физика планет и малых тел Солнечной системы . ... Федеральное государственное бюджетное учреждение науки Институт космических исследований Российской академии наук (ИКИ РАН) - головной академический институт по исследованию и использованию космического пространства в интересах фундаментальных наук. ... Одиннадцатая ежегодная конференция "Физика плазмы в солнечной системе" . ... ФГБУН Институт космических исследований Российской академии наук (ИКИ РАН) . ...

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• A Brief History of Magnetospheric Physics Before the Spaceflight Era

Next: Emission-line galaxies Up: The Hamburg/SAO Survey for Previous: Data reduction . ... Among them 128 are new or confirmed emission line galaxies, 6 are quasars (all with redshifts in the range 2.93 to 3.35) and 23 are galaxies without emission lines (only 5 of them have good enough S/N ratio to identify absorption features and to measure redshifts). ... Emission-line galaxies . ... Non emission-line objects . Absorption line galaxies . Stellar objects . Non-classified objects . ...

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• Up-date RC-sources Spectra
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... Galaxies 99 Cosmic background with model of cloudy interstellar medium Yu. ... Figure 1: Averaged spectrum of the cosmic background I f in frequency range 0.25 200 MHz for the Galactic poles. ... First interpretation of the cosmic noise background spectrum at broad band frequency range 0.25 200 MHz with a model of the cloudy interstellar medium ISM is presented here. ... Synthesized background spectra I f for regions of the Galactic poles at the frequency range 0.25 200 MHz is presented in Fig. ...

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• http://www.gao.spb.ru/english/as/j2014/presentations/filippova.pdf

... 13th European VLBI Network Symposium . and Users Meeting . on September 20-23, 2016. ... 13th European VLBI Network Symposium and Users Meeting on September 20-23, 2016. ... Year book "Ephemerides of Minor Planets for 2016" on-line . ...

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• Information for Authors of Articles

... The presence of solid­state emission bands is compared to other indicators of circumstellar material, such as Hff emission, optical variability and sub­mm continuum fluxes. ... However, a strong dependence on spectral type of the central star seems to be present: stars with spectral type earlier than B9 show either amorphous silicate in absorption or infrared spectra dominated by PAH emission, whereas more than 70% of the stars of later spectral type show silicate emission. ...

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• The past, present and future appearances of the Refsdal supernova | ESO
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Main Program Travel Where to go in Moscow Information . ... The 2014 year marks the 100th anniversary of Yakov Zeldovich . ... John Carlstrom (University of Chicago) . ... Lyman Page (Princeton University) . ... The conference will be held at the Space Research Institute (IKI) in Moscow, Russia, on June 16-20, 2014 . ... International Conference: Cosmology and High Energy Astrophysics (Zeldovich-90) 20-24 Dec 2004, Moscow, Russia . ... 2014 Space Research Institute, Moscow Русская версия ...

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31. Origin of the internal structures in HL Tauri jet (HH 151)

32. ST-ECF Grism Spectrum Software for NICMOS Grism Data

33. Large_Scale Emitting Chains

34. Armagh Observatory

35. http://www.astro.louisville.edu/software/sbig/archive/xmccd-2.1/TODO

36. Баллистический центр Института прикладной математики им. М.В.Келдыша РАН

37. http://www.atnf.csiro.au/research/masermeeting/web_papers/523_Rudnitskij.pdf

38. Marat Abubekerov - Curriculum Vitae

39. Home Page