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201. http://curl.sai.msu.ru/mass/download/doc/massug.pdf
MASS Software Version 2.04 User Guide V.Kornilov, N.Shatsky, O. Voziakova Decemb er 30, 2003 Contents 1 MASS software op eration overview 1.1 Main features of measurement pro cess with MASS instrument . ... 2 Installation, tuning and startup 2.1 Installation of the MASS software Turbina 2.2 Editing the configuration file . ... 4.2 Output data in MASS Software . ... 4.2 Output data in MASS Software The output of Turbina program op erating the MASS device is directed to an ASCI I file called mass-file. ...
[ Текст ]  Ссылки http://curl.sai.msu.ru/mass/download/doc/massug.pdf -- 297.2 Кб -- 18.01.2004
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202. http://www.princetonastronomy.org/newsletters/04_2003sidereal.pdf
Chairman: Mark Lopez (609) 393-2565 mal455@earthlink.net Editor: Victor Belanger (609) 448-8598 vic@apink.com Assistant Director: John Miller (609) 252-1223 jcm726@earthlink.net Volume 32 From The Program Chairman I know that most of you are regular readers of Sky Telescope and Astronomy magazines, and like myself, you are also frequent visitors to NASA's Astronomy Picture of the Day web site ... He began astro-imaging in1996 with a 10" Schmidt Cassegrain and a CCD camera. ...
[ Текст ]  Ссылки http://www.princetonastronomy.org/newsletters/04_2003sidereal.pdf -- 1157.6 Кб -- 27.04.2003
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203. http://sn.sai.msu.ru/~sil/preprints/n5055.ps.gz
... Kinematics and stellar population properties in the center of nearby Sbc galaxy NGC 5055 are studied with the Multi­Pupil Spectrograph of the 6 m telescope of the Special Astrophysical Observatory of Russian Academy of Sciences (SAO RAS). ... We have found a resolved chemically distinct core in NGC 5055, with the magnesium­enhanced region shifted by 2. ## 5 (100 pc) to the south­west from a photometric center, toward a kinematically identified circumnuclear stellar disk. ... 22 ± 6 Ionized gas 1. ...
[ Текст ]  Ссылки http://sn.sai.msu.ru/~sil/preprints/n5055.ps.gz -- 187.0 Кб -- 03.06.2002
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204. source comment
. Comment on J0319+4130 . Our image does represent the main source structure. However, due to the limited u-v coverage, it does not have as high fidelity as other known images, such as the one at 5 GHz by Romney et al. (1995). VLBApls home page . Last modified: 16 Oct 2000
[ Сохраненная копия ]  Ссылки http://www.vsop.isas.ac.jp/VLBApls/J0319+4130.comment.htm -- 1.5 Кб -- 16.10.2000
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