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). · 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 Con