Science, Volume 293John Michels (Journalist) American Association for the Advancement of Science, 1717 |
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Page 1782
... Galaxy in- teractions and mergers are much more likely when the density of galaxies is in- creased . Such interactions can disrupt the stability of galaxy disks , resulting in rapid was sufficiently long to allow atomic gas masses as ...
... Galaxy in- teractions and mergers are much more likely when the density of galaxies is in- creased . Such interactions can disrupt the stability of galaxy disks , resulting in rapid was sufficiently long to allow atomic gas masses as ...
Page 1799
... galaxy ~ 18 h65-1 kpc to the southwest . We christened the HI - selected spiral galaxy A2218 - H1 . The J2000 coor- dinates of A2218 - H1 are a = 16 : 33 : 58.5 and 8 = +66 : 10 : 06 . From the imaging observations we infer that the ...
... galaxy ~ 18 h65-1 kpc to the southwest . We christened the HI - selected spiral galaxy A2218 - H1 . The J2000 coor- dinates of A2218 - H1 are a = 16 : 33 : 58.5 and 8 = +66 : 10 : 06 . From the imaging observations we infer that the ...
Page 1800
... galaxy enters the ICM . The position of A2218 - H1 is about 11 arc min west from the central super giant elliptical ( cD ) galaxy , which also marks the peak of the x - ray profile . This separation translates to a projected distance of ...
... galaxy enters the ICM . The position of A2218 - H1 is about 11 arc min west from the central super giant elliptical ( cD ) galaxy , which also marks the peak of the x - ray profile . This separation translates to a projected distance of ...
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