... It is a panoramic integral-field spectrograph for ``understanding the formation and evolution of elliptical and lenticular galaxies and of spiral bulges from 3D-observations'' ( http://www.strw.leidenuniv.nl/sauron ). ...
... It is a panoramic integral-field spectrograph for "understanding the formation and evolution of elliptical and lenticular galaxies and of spiral bulges from 3D-observations" (http://www.strw.leidenuniv.nl/sauron). ...
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Ссылки http://www.adass.org/adass/proceedings/adass03/reprints/O5-2.pdf -- 1213.7 Кб -- 27.08.2004 Похожие документы
... It now established that galaxies are not "island universes", but rather interact with each other in pairs or in small or big ... Interactions can form spirals, bars, warps, rings and bridges. ...
... Introduction It now established that galaxies are not "island universes", but rather interact with each other in pairs or in ... Interactions can form spirals, bars, warps, rings and bridges. ...
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Ссылки http://www.adass.org/adass/proceedings/adass03/reprints/P7-8.pdf -- 103.9 Кб -- 27.08.2004 Похожие документы
... Using a web interface, the user can select the number of galaxies to be modeled, and for each, the model type, number of ... Models include, from NEMO, Plummer, baredisk, exponential disk, homogeneous sphere, polytrope and spiral. ...
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Ссылки http://www.adass.org/adass/proceedings/adass02/reprints/D10.pdf -- 67.9 Кб -- 11.03.2003 Похожие документы
... Using a web interface, the user can select the number of galaxies to be modeled, and for each, the model type, number of ... Models include, from NEMO, Plummer, baredisk, exponential disk, homogeneous sphere, polytrope and spiral. ...
... Structure and kinematics of our Galaxy · Shape and rotation of the bulge, disk and halo · Internal motions of star forming regions, clusters, etc · Nature of spiral arms and the stellar warp · Space motions of all Galactic satellite systems 2. ...
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Ссылки http://www.adass.org/adass/proceedings/adass03/reprints/O8-2.pdf -- 199.4 Кб -- 27.08.2004 Похожие документы
... testing for completeness in sampling (whether the expected structure is revealed as spiral or filamentary), (3) testing whether resolution is achieved (in the cores of galaxies), (4) the creation of maps with resolution higher than the physical resolution ...