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1. High-resolution Near-infrared Study of the Deeply Embedded Young Stellar Object
... High-resolution Near-infrared Study of the Deeply Embedded Young Stellar Object S140 IRS 3 . ... P22P We explore the structures immediately surrounding the high-mass young stellar object S140 IRS 3 within the L1204 molecular cloud. ... The S-shaped structure of this feature can be well reproduced by a model assuming a precessing outflow from IRS 3a. Furthermore, we find several elongated features pointing away from IRS 3 in a southern direction. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2001/preibisch_2001.html -- 12.1 Кб -- 02.10.2012
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2. FIND/ROMAFOT
Next: ANALYSE/ROMAFOT Up: The Interactive Path Previous: The Interactive Path . FIND/ROMAFOT frame [cat_tab] . This command works exactly like SELECT/ROMAFOT and therefore needs no detailed explanation. The only difference is that FIND/ROMAFOT , designed to select many stars, stores the positions of the objects in a catalogue table which has a different structure than then the intermediate table created by SELECT/ROMAFOT . This table serves as as input for the command ANALYSE/ROMAFOT . ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/94NOV/vol2/node104.html -- 3.2 Кб -- 23.02.1996
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3. A unique isolated dwarf spheroidal galaxy KKR25
... We present a photometric and spectroscopic study of the unique isolated nearby galaxy KKR25. The isolated dwarf spheroidal (dSph) galaxy KKR25 was discovered by Karachentseva, Karachentsev Richter (1999, A , 135, 221) during the search of dwarf galaxies in the direction of the Local Void. In spite of its isolation KKR 25 has no gas and looks like a normal dwarf spheroidal system. ... This is the first known planetary nebula in a dwarf spheroidal galaxy outside the Local Group. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/Doc-en/SciNews/2012/Makarov/ -- 5.8 Кб -- 02.10.2012
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4. Informational system "Evolution of RG"
The project of the informational system creation on the problem of evolution of radio galaxies, as a part of the "Big Trio" project aimed on studing of distant radio galaxies, is designed. This system allows a user to operate with simulated curves of spectral energy distributions (SED) to estimate ages and redshifts by photometry data. Authors use SEDs of several models for different types of galaxies. ... The HTTP and e-mail access is organized to this system. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/sed/ -- 4.7 Кб -- 15.07.2001
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