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http://www.atnf.csiro.au/research/masermeeting/web_papers/305_DeBuizer.pdf.
http://www.atnf.csiro.au/research/masermeeting/web_papers/305_DeBuizer.pdf.
1. The Spectral Energy Distribution and Mass-Loss Rate of the A-Type Supergiant
... The measured bolometric flux and corrected NPOI angular diameter yield an effective temperature of 8600+/-500 K. Least-squares comparisons of synthetic spectral energy distributions from 1220 Г: to 3.6 cm with the observations provide estimates for the effective temperature and the mass-loss rate of ~=8400+/-100 K and (8+/-3)Г-10-7 Msolar yr-1, respectively. ... ADS Citation Query . citations = 34 . citations vs. year [year,citations] . ...
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Ссылки http://www.stsci.edu/~kgordon/papers/2002ApJ...570..344A.html -- 4.7 Кб -- 21.01.2016
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2. Distributed Software for Observations in the Near Infrared
... We have developed an integrated system that performs astronomical observations in Near Infrared bands operating two-dimensional instruments at the Italian National Infrared Facility's ARNICA and LONGSP . ... The user interface is organized as widget-based X11 client. ... 1993; Di Giacomo et al. 1993). ... Moreover, if the interprocess communication interface includes support for networking, the software immediately becomes network distributed software. ... DESQview/X User Guide 1993, Quarterdeck . ...
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Ссылки http://www.adass.org/adass/proceedings/adass94/gavryusevv.html -- 9.9 Кб -- 03.11.2000
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3. Initial Distributions of Binary Parameters
Next: Star Formation Rate and Up: No Title Previous: Calculation of Evolutionary Tracks . To start calculations, we choose the distributions of the initial binary parameters: the mass of the primary ZAMS component, , binary mass ratio, , orbital separation a . ... whereas the mass ratio distribution is not. ... The zero assumption often made is that the mass ratio distribution has a flat shape, that is binaries with a high mass ratio occur as frequently as those with equal masses. ...
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Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node39.html -- 14.1 Кб -- 26.02.1997
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4. The spectral energy distribution of PKS 2004-447: a compact steep-spectrum
An investigation of the spectral energy distribution (SED) of the compact steep-spectrum (CSS) source and possible radio-loud narrow-line Seyfert 1 galaxy (NLS1), PKS 2004-447, is presented. ... Analysis of a non-contemporaneous, low-resolution optical spectrum suggests that the narrow-line region (NLR) is much more reddened than the X-ray emitting region suggesting that the gas-to-dust ratio in PKS 2004-447 may be very different than in our own Galaxy. ...
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Ссылки http://www.atnf.csiro.au/people/Matthew.Whiting/papers/html_abstracts/b2004_abs.html -- 5.6 Кб -- 26.12.2007
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5. http://www.mrao.cam.ac.uk/~krause/KA-nam-2006-poster.pdf
Multiphase Turbulence in Extragalactic Jet Cocoons Martin Krause Paul Alexander Cavendish Laboratory, University of Cambridge The observations ( Alignment effect ) · Radio galaxies at redshift 0.5 show associated optical emission : emission lines + rest frame blue continuum, correlations of many properties are evidence for the interaction · ... Note the pronounced peak at 14,000 K. The system energy reduces much faster, the more cold mass added. ... No cool gas appears in the control run. ...
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Ссылки http://www.mrao.cam.ac.uk/~krause/KA-nam-2006-poster.pdf -- 847.4 Кб -- 31.03.2006
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6. Comments on: chi-square distribution [Eqn] By: Alex By: vlk By: aneta By: aneta
http ://hea-www.harvard.edu/ AstroStat /slog/2008/eotw-chisq- distribution / Weaving together Astronomy+Statistics+Computer Science+Engineering+Intrumentation, far beyond the growing borders Fri, 01 Jun 2012 18:47:52 +0000 hourly 1 http ://wordpress.org/?v=3.4 http ://hea-www.harvard.edu/ AstroStat /slog/2008/eotw-chisq- distribution /comment-page-1/#comment-308 Alex Sun, 27 Jul 2008 01:52:08 +0000 http ://hea-www.harvard.edu/ ... Thanks, Aneta, very useful comment. ...
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Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/2008/eotw-chisq-distribution/feed/index.html -- 7.5 Кб -- 04.02.2013
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7. http://www.sao.ru/cats/~satr/RFSymp/abs/17_Korzhavin.ps
ESTIMATIONS OF EFFECTIVE HEIGHT, SIZE AND BRIGHTNESS TEMPERATURE OF SOLAR CYCLOTRON SOURCES A.N. Korzhavin, T.I. Kaltman Special Astrophysical Observatory of RAS, SaintPetersburg, Russia arles@mail.ru The modeling of microwave emission from a spotassociated cyclotron source was done to refine the method of estimations of e#ective brightness temperature, size and height above photosphere in the processing of RATAN600 observations. ...
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Ссылки http://www.sao.ru/cats/~satr/RFSymp/abs/17_Korzhavin.ps -- 50.0 Кб -- 09.10.2006
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