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Download Internal Kinematics and Dynamics of Galaxies by Vera C. Rubin (auth.), E. Athanassoula (eds.) PDF

By Vera C. Rubin (auth.), E. Athanassoula (eds.)

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Naval Obs. XX, part. , 1982, Astrophys. S. , 1978, Ph. D. , 1981a, Astron. J. , 1981b, Astron. J. , 1977a, Astron. Astrophys. , 1977b, Astron. Astrophys. , 1979, Astron. Astrophys. , 1980, Astron. Astrophys. , 1981, Astron. Astrophys. H, 1982, Astrophys. J. , 1982, Astron. Astrophys. , 1942, Ann. Obs. Lund No. , 1959, Astrophys. J. , 1963, Astrophys. J. , Astrophys. J. , 1982, Astrophys. J. , 1982, Astron. , 1981, Astrophys. J. , 1981, Astron. Astrophys. , 1982, Astron. J. S. S. S. S. , 1971, Astron.

G. a constant MIL for the disk, one still has the freedom to choose specific disk and halo models which all fit the handful of independent data points well. 8 which fits the observed rotation curve reasonably well. L)disk. Clearly we need other ways to determine the properties of the massive halo, if it exists, than rotation curves alone. , 1971, Publ. S. Naval Obs. XX, part. , 1982, Astrophys. S. , 1978, Ph. D. , 1981a, Astron. J. , 1981b, Astron. J. , 1977a, Astron. Astrophys. , 1977b, Astron.

Dent University of Manchester, Nuffield Radio Astronomy Laboratories, Jodrell Bank, Macclesfield, Cheshire, SKll 9DL England The galactic nucleus contains the largest concentration of dense molecular clouds in the Galaxy. A new survey of the region has been carried out recently at Jodrell Bank in the 1667 and 1665 MHz lines of OH (Cohen 1981). The OH lines appear primarily in absorption against the galactic continuum background. The survey reveals many new clouds within the previously known nuclear concentration, and also a more extensive outer distribution of clouds extending to projected distances of ±l kpc from the centre.

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