Astronet Поиск по астрономическим сайтам English Russian
       
        Точная форма слов   О проекте   Сайты   Справка
Найдено документов: 313261 (223 сайтов) ---- Время поиска: 0.95сек.   

В начало ] Пред. | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12

Показаны документы, содержащие фрагменты текста из документа
http://news.cosmoport.com/2009/08/21/1.htm.

221. http://sn.sai.msu.ru/~sil/preprints/leo3.pdf
... The kinematics, structure, and stellar population properties in the centers of two early-type spiral galaxies of the Leo Triplet, NGC 3627 and NGC 3623, are studied by means of integral-field spectroscopy. ... In the center of NGC 3627 we observe noticeable gas radial motions, and the stars and the ionized gas in the center of NGC 3623 demonstrate more or less stable rotation. ... In this work we consider two nearby early-type spiral galaxies belonging to the famous Leo Triplet, NGC 3623 and NGC...
[ Текст ]  Ссылки http://sn.sai.msu.ru/~sil/preprints/leo3.pdf -- 470.1 Кб -- 04.10.2005
Похожие документы

222. http://www.vista.ac.uk/Files/docs/VISTA_in_eso-messenger-no117.pdf
T HE V I www.vista.ac.uk V ISTA'S ISIBLE & NFRARED S UR VEY T ELESCOPE FOR A STRONOMY .R 1.65DEGREE DIAMETER INFRARED FIELD OF VIEW FEEDS A APID DEEP IR 4- METRE PRIMARY MIRROR AND MEGAPIXEL OBJECTS FOR FOLLOW-UP WITH VLT, AND DIRECTLY STUDY A WIDE VARIETY OF ASTRONOMICAL TOPICS (0.34 PIXEL ) CAMERA (0.85­2.3µm) 64 IMAGING SURVEYS WILL BOTH SELECT . ... As an ESO telescope, VISTA and its large surveys will now be fully exploited by the whole ESO community. ... VISTA Figure 9: Telescope support base. ...
[ Текст ]  Ссылки http://www.vista.ac.uk/Files/docs/VISTA_in_eso-messenger-no117.pdf -- 919.4 Кб -- 14.06.2012
Похожие документы

223. http://www.2dfquasar.org/Papers/2002MNRAS.337..275C.pdf
... 337, 275­292 (2002) The correlation of line strength with luminosity and redshift from composite quasi-stellar object spectra S. M. Croom,1 K. Rhook,1 E. A. Corbett,1 B. J. Boyle,1 H. Netzer,2 N. S. Loaring,3 L ... We measure highly significant Baldwin effects for most broad emission lines (C IV 1549, C III] 1909, Mg II 2798, H ,H ) and show that they are predominantly caused by correlations with luminosity, not redshift. ... The correlations of log W with log(1 + z ) for each line. ...
[ Текст ]  Ссылки http://www.2dfquasar.org/Papers/2002MNRAS.337..275C.pdf -- 831.9 Кб -- 04.03.2004
Похожие документы

В начало ] Пред. | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12

Rambler's Top100 RFBR Яндекс цитирования