Massive evolved stars can produce large amounts of dust, and far-infrared (IR) data are essential for determining the contribution of cold dust to the total dust mass. Using Herschel, we search for cold dust in three very dusty massive evolved stars in the Large Magellanic Cloud: R71 is a luminous blue variable, HD 36402 is a Wolf-Rayet triple system, and IRAS05280-6910 is a red supergiant. ... ADS ] . ADS Citation Query . ... 2010,1][2011,6][2012,2][2013,6][2014,4][2015,2] . ...

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• Dust Masses, PAH Abundances, and Starlight Intensities in the SINGS Galaxy
• Simulation Parameters
• HST this week: 049

... Launch of International Crew VC-4 by Soyuz TMA-1 manned spacecraft; . ... Implementation of experiments ( Acoustoka-M , Diurez , Biotest , Biodegradation , Uragan , Diatomeya ) under the Russian program and experiments ( "VITAMIN D" , "RHOSIGNAL" , "RAMIROS" , "MESSAGE" , "GCF-B" , "PROMISS" , "CARDIOCOG" , "NEUROCOG" , "SYMPATHO" , "VIRUS" , "SLEEP" , "DCCO" , "ZEPGRID" , "NANOSLAB" , "COSMIC" , "LSO-B" , "EDUCATION" ) under ODISSEA commercial program onboard the International Space Station; . ...

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• S.P.Korolev RSC Energia - MIR ORBITAL COMPLEX
• S.P.Korolev RSC Energia - LAUNCHERS
• S.P.Korolev RSC Energia - SCIENTIFIC-EDUCATIONAL PROGRAM

Proposal Identification No.: A1914 Date Received: 2004-Feb-01 19:49:03 Technical Page Proposal Type: General Category: Sub-Category: Observation Category: Total Time Requested: Prop osal Title: ABSTRACT: Regular Astronomy Spectroscopy Extragalactic 7.5 Hours The HI properties of the faintest Blue Compact Dwarf, SA 68 6597 We prop ose to measure the HI content and linewidth of SA 68-6597 in order to b etter constrain its total mass and p otential for future star formation. ...

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• http://www.naic.edu/vscience/schedule/tpfiles/JanchestagT1998tp.pdf
• http://www.naic.edu/vscience/schedule/tpfiles/JanchestagT1998tp.ps
• http://www.naic.edu/vscience/schedule/tpfiles/PisanotagA1914tp.ps

... The star formation rate (SFR) of the current SF episode can be estimated from the total H luminosity. ... For the derived total flux F (H )=5.8 erg s -1 cm -2 we obtain a total H luminosity of 10 39 erg s -1 . ... The total mass of ionized gas can be obtained from the average mass density inside the H II region and its volume. An average mass density corresponding to the average electron density of 1 cm -3 within a volume with a diameter of 0.5 kpc yields a total ionized gas mass of 10 6 . ...

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• H I and dynamical mass
• Millimeter continuum of extragal. sources, Steppe et al.
• Summary of the present status of the survey

Astronotes Armagh Planetarium's Stellar Blog! ... March . ... Posted on May 20, 2015 | No Comments If you missed the Lyrids meteor shower in April, starting of May you had another chance to see some shooting stars as the Eta Aquarids meteor shower peaks on the [ ] . Continue Reading.. ... No Comments In association with BBC Stargazing Live 2015 and the Northern Ireland Amateur Astronomical Society (NIAAS) Armagh Planetarium is opening its doors for a free open evening on Tuesday 24th of [ ] . ...

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• observing | Astronotes - Part 2
• stars | Astronotes
• Orion | Astronotes - Part 2

... The relationship of the mass and the observed galactocentric distance R -- (a), and that of the mass and the total dissipation velocity n taken from Gnedin, Ostriker (1997) -- (b). The dotted line in diagram (a) shows the "cone of survival" according to the paper by Surdin and Arkhipova (1998) . ... The solid line is a regression stright line for the main sequence of clusters, and the dotted line parallel to it separates the sequence of clusters of anomalously small mass shown by open triangles. ...

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• Vladimir Marsakov Publication List

... Thermogravimetric and differential thermal analysis . ... TOF-SIMS analysis . Total conductivity, Seebeck coefficient and ion transference number measurements in controlled atmos . ... Processing of ceramic materials, electrode systems and electrochemical cells . ... SIMS analysis is based on exposure of the sample surface with primary ions possessing some definite energy, which is partially consumed by the sample and induces emission of sН-called secondary ions. ... Spatial resolution: 60 nm . ...

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• About BTA
• The VII Asian-Pacific Astronomy Olympiad: ages table
• Laboratory of spectroscopy of defect structures ISSP RAS

... 2006 . ... Comparison of total ozone distribution in the high latitudes of both hemispheres SCAR XXIX Open Science Conference, 2006, 12-14 July, Hobart, Australia - Abstract Volume. ... Analyses of spectra, stability and eigenmode transverse small-scale oscillations in the inner Earth magnetosphere. 6th Open Conference of Space Projects Evpatoriya, September 2006, Abstracts . ... Ps6 pulsations in the Earth magnetosphere. 5th Open Conference of Space Projects Evpatoriya, September 2005, Abstracts . ...

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• Mykola I. Dzubenko

... citations = 1930 (533 on first author papers). Ї h-index=25 Conferences attended Multiwavelength Views of the ISM in High-Redshift Galaxies , Santiago, Chile, June 2011 (co-chair of the LOC) Galaxies , Near and Far, Villa Aureli, Perugia, Italy, May 2011 ( invited talk ) Diffuse Relativistic Plasmas, Bangalore, India, March 2011 ( invited talk ) COSPAR 2010, Cosmic Feedback, Bremen, Germany, July 2010 ( invited talk ) Powerful Radio ...

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• ESO - E-ELT Science Instrumentation, 25 Feb - 1 Mar 2013
• Astronomical Events | ESO
• European ALMA antenna brings total on Chajnantor to 16 | ESO Australia

... Here I will briefly describe some of the key surveys taking place, the distinction between cosmology and galaxy evolution studies and an update of where we are in terms of mapping the Universe (and whether weтАЩre likely to run out of Universe anytime soon). IтАЩll then focus on science from the GAMA project, very briefly summarising some of the key results from the first 100 papers, before focussing on where we are with the mass and energy census in the Universe. ...

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• http://www.mso.anu.edu.au/pfrancis/phys1101/Lectures/L02/lecture02.pdf
• Index of /~akarakas/stellar_yields
• Dougal Mackey - CV

MINUTES of the RadioAstron Teleconference on February 21, 2006 V. Slysh chaired the teleconference. ... Engineering model of the MFS (18-26 GHz) on-board receiver has been fabricated, and it is now under the testing in the ASC. The flight model is expected in April 2006. ... Operational time of 18-cm receiver was prolonged till the end of 2007 (as a launch date).The flight model of the 92-cm receiver will be delivered to the ASC in May 2007. ...

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• RadioAstron main page, english version
• Description of the RadioAstron project, english version
• RadioAstron meeting

... Image Quality of the VLT . Total Optical Control . First light for the ESO VLT unit telescope 1 occurred during the workshop. ... The image shown (Figure 1 ) here was obtained with the VLT on May 16, 1998, in red light (R band), i.e. while the mirror was still uncoated. ... In this diagram (FIgure 2), the measured image quality of the VLT UT1 astronomical images is plotted versus the ``seeing", as measured by the Seeing Monitor, a small telescope also located on top of the Paranal Mountain. ...

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... This is a preliminary summary of the event on November 24, 1996, considered during the INTERBALL Workshop in Kiljavanranta, Finland, February 1998. ... Pronounced plasma sheet thinning (Bz decrease) . ... Particle burst observed inside the Polar Cap and in tail lobes . A short burst of particles detected by the Auroral Probe particle detectors during the Polar Cap crossing at 21:45 UT, almost simultaneously with the Tail Probe detectors registration of the particle burst inside the North Lobe. ...

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• Lidar homepage - Instrument Information
• Interball Workshop Programme
• Space Research Institute (IKI) Seminar

Twilight observations with MASS/DIMM B. Safonov Sternberg Astronomical Institute Moscow State University Comprehensive Characterization of Astronomical Sites, 2010 B. Safonov (Moscow State University) Twilight observations with MASS/DIMM SITE 2010 1 / 17 Why observe in twilight with MASS/DIMM? ... ASM includes 3 devices sensitive to background: guider, DIMM and MASS. B. Safonov (Moscow State University) Twilight observations with MASS/DIMM SITE 2010 2 / 17 Background in guider. ...

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Laboratory of Stellar Physics . ... A study of close binaries with black holes, neutron stars and white dwarfs. ... A study of SS433 - the massive close binary with a black hole in the regime of supercritical accretion . ... A search for intermediate-mass black holes (IMBH). The black holes which are not supermassive black holes observed in quasars, and which were formed not in massive stars. ... A search for new magnetic stars, new CP stars, measurements of magnetic fields in stars . ...

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• Radio Astronomical Seminars, 1998
• Olga Maryeva homepage
• Vitaly Goranskij, SAI/Moscow Univ.

. Full-Text Search . Latest . Statistics . arXiv.org . > . astro-ph . recent . find . SAI VO . Search sort results by Date Relevance . Use logical operators AND , OR , NOT and round brackets to construct complex queries. Whitespace-separated words are treated as AND ed. Show 10 50 100 articles per page in Full Compact mode . Normalized to: Mass, D. 1 article(s) in total . 2 co-authors. Median position in authors list is 3,0 . Co-author(s): . Ignace, R. - . Oskinova, L. M.. SAI VO | Astronet | SAI MSU .

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. July 14 . November 8 . Previous slide . Next slide . Back to first slide . View graphic version .

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• Algorithm

... Experimental base . ... The experimental base of the investigations is the topside sounding data obtained on board of the Intercosmos-19 and Cosmos-1809 satellites. ... It carried on board the following scientific payload: satellite ionospheric station for radio sounding of ionosphere (IS-338) and apparatus for the measurements of low-frequency electromagnetic field (VLF-2ME), electric component of high-frequency field (AHF-2K), electron temperature (KM-3), and spectrometer of photoelectrons (SF3-M)...

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• November 2004
• TOTAL SOLAR ECLIPSE OF MARCH 9, 1997
• CMEs and Space Weather

... We consider the astrophysical evolution of the Galaxy over large time scales, from early stages (an age of ~10 8 yrs) to the end of traditional stellar evolution (~10 11 yrs). ... In the model considered, the basic stages of Galactic evolution are as follows. ... Essentially all other basic parameters of the Galaxy vary little. ... The final "stellar epoch" in the life of the Galaxy is completed ~10 13 yrs after its formation, when the evolution of the least massive stars comes to an end. ...

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TIME EVENT # EVENT DATE DATE START - END (UT) 001 28 February 1942 420228 002 07 March 1942 420307 003 25 July 1946 460725 004 19 November 1949 491119 005 23 February 1956 560223 020000 - 030000 006 31 August 1956 560831 110000 - 120000 007 17 July 1959 590716 220000 - 240000 008 04 May 1960 600504 090000 - 100000 009 03 September 1960 600902 230000 - 240000 010 12 November 1960 601112 120000 - 130000 011 15 November 1960 601115 010000 - ...

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• http://www.wdcb.ru/stp/data/Images_of_Magnetograms/MGD/MGD2001/
• http://www.wdcb.ru/stp/data/Images_of_Magnetograms/MGD/MGD1998/
• http://www.wdcb.ru/stp/data/Images_of_Magnetograms/MGD/MGD2000/