... as plumes, tails, TDGs, regions with very different chemical abundances inside galaxies, perturbed kinematics of the ionized gas or lack of neutral hydrogen gas, confirming the hypothesis that interaction with or between dwarf ob jects triggers the star ...
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Ссылки http://www.atnf.csiro.au/people/Angel.Lopez-Sanchez/proceedings/SEA_Barcelona_2006_lopez-sanchez.pdf -- 394.2 Кб -- 30.10.2006 Похожие документы
... as plumes, tails, TDGs, regions with very different chemical abundances inside galaxies, perturbed kinematics of the ionized gas or lack of neutral hydrogen gas, confirming the hypothesis that interaction with or between dwarf ob jects triggers the star ...
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Ссылки http://www.atnf.csiro.au/people/Angel.Lopez-Sanchez/proceedings/angelrls_granada07.pdf -- 228.5 Кб -- 14.01.2008 Похожие документы
... By contrast, neutral hydrogen is primordial, and the 21 cm line has such a low excitation temperature that the ionizing extragalactic background radiation is sufficient to maintain its excitement. ...
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Ссылки http://www.atnf.csiro.au/research/conferences/2014/ThePeripheryOfDisks/POD_Conference_Program_v5.pdf -- 102.5 Кб -- 11.11.2014 Похожие документы
... slower expanding AGB envelope and are able to excite the H #tex2html_wrap_inline428# emission, and in the young planetary nebula phase ultraviolet radiation from the hot, central star ionizes the inner cavity and excites the molecular hydrogen in the PDR ...
... Turbulence in the warm ionized interstellar gas - Dr Marijke Haverkorn Colloquium. ... the neutral hydrogen line and full-polarization 1420 MHz continuum . ... fluctuations in warm ionized gas in the Galactic spiral arms. More information . ...