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41. The Structure and Composition of High Redshift Radio Galaxies
... Keck spectropolarimetry, giving spectral coverage from Ly- to beyond CIII], and HST imaging of a sample of powerful radio galaxies with has been obtained. ... This is a short progress report on a rather extensive programme we are carrying out to study the structure and composition of high redshift radio galaxies (HzRG) -- and, by implication, the host galaxies of radio quasars -- using observations in the optical, IR and mm bands. ... An example of the NICMOS and WFPC 2 imaging is shown in Figure 2 ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node33.html -- 19.1 Кб -- 12.06.2006
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42. Supernova 1999bg in IC 785
This page is devoted to information on Supernova 1999bg in IC 758 . ... Information on the original web pages for many of these images can be found on the Supernova links web page. 1999bg is another discover by the Lick Observatory Supernova Search who have been very prolific over the past year but have had a bit of a lull lately. ... AUDE has a 1999bg page in French [ Translate ] . M1 Supernova search has a 1999bg page in Spanish [ Translate ] . Seiichi Yoshida has a 1999bg images page . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/mirrors/isn/snimages/sn1999/sn1999bg.html -- 9.4 Кб -- 22.12.2007
[ Сохраненная копия ]  Ссылки http://www.rochesterastronomy.org/SNIMAGES/sn1999/sn1999bg.html -- 9.6 Кб -- 19.04.2014
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43. http://www.puldb.ru/jenam_2011/PUB_JENAM_2011/shakht_1.pdf
Central Bodies Masses of Selected Globular Clusters N.A.Shakht, A.A.Kiselev, Yu.N.Gnedin and E.A.Grosheva. The Main Astronomical (Pulkovo) Observatory RAS 47 Tuc ­NGC 104 RA 00 24 .1 Dec -72° 04 .9 Size = 30.9 mvis + 4. 0 m D from = 12,1 kpc, h m Cen - NGC 5139 NGC 6397 (Ara) RA 17 h40.m7 Dec -53o 40'.4 Size = 31',0 mvis + 5,3m D from =2.3 kpc RA 13h 26m .8 Dec -47° 28 6 Size = 36.3 m vis +3. 7 m D from =15.8 ±1.1 kpc, 12109 years, Age: 10109 years, (13.4 ± 0.8)109 years. ...
[ Текст ]  Ссылки http://www.puldb.ru/jenam_2011/PUB_JENAM_2011/shakht_1.pdf -- 678.1 Кб -- 05.01.2013
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44. http://www.gao.spb.ru/english/as/j2014/presentations/mosenkov.pdf
Decomposition of Galaxy Images and Galaxy Rotation Curves Mosenkov A.V.*^, Savchenko S.S.*, Sotnikova N.Ya.* ... The DECA (DEComposition Analysis) code is designed to investigate images of galaxies in an automatic regime (using the simple 'bulge+disc' model) as well as in manual mode for more detailed images and/or for multicomponent structures. ... The GRCF package was created for performing the galaxies rotation curve decomposition using the models of the bulge, the disc, and the dark halo. ...
[ Текст ]  Ссылки http://www.gao.spb.ru/english/as/j2014/presentations/mosenkov.pdf -- 612.3 Кб -- 30.09.2014
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45. http://www.atmob.org/about/observing/awards/files/galaxy_instructions_2011-02-01.pdf
ATMoB "Galaxy Observing Award " Guidelines Purpose: To promote observing among the membership of the Amateur Telescope Makers of Boston through participation in the Galaxy Observing Awards program. ... Examples of elliptical galaxies: M49, M59, M60, M87, NGC 4125. Limiting Magnitude Assessment: Spirals: A spiral galaxy consists of a flattened disk, with stars forming a (usually two-armed) spiral structure, and a central concentration of stars known as the bulge. ...
[ Текст ]  Ссылки http://www.atmob.org/about/observing/awards/files/galaxy_instructions_2011-02-01.pdf -- 27.4 Кб -- 21.02.2011
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46. MILLIMETRON
... The project assumes creation of an international space observatory - the interferometer "Earth - Space - Space" in order to perform of astronomical investigations in millimeter, submillimeter and infrared regions with extremely high sensitivity (to a few nanoJanskies units of flux density in continuum spectrum) and extremely high angular resolution (to a parts of microsecond of arc or, possibly, nanosecond). ... radio-interferometric channels of the system "Space - Space", region 0.2 - 3 mm; . ...
[ Сохраненная копия ]  Ссылки http://www.asc.rssi.ru/submillimetron/mm/default.htm -- 10.5 Кб -- 05.04.1999
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