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- W201306114 abstract "The dynamics of the outer regions of elliptical galaxies is still poorly known. Their lack of gas means that it is not possible to use the usual optical and 21cm emission lines to determine the kinematics out to large radii, and the faintness of their stellar body means that data calculated using absorption lines are limited to the inner part of the galaxy. It is only by measuring the kinematics out to several optical scalelengths that one gets any unambiguous measure of the dark halo properties (Kent 1986)." @default.
- W201306114 created "2016-06-24" @default.
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- W201306114 date "2003-01-01" @default.
- W201306114 modified "2023-09-24" @default.
- W201306114 title "Theoretical Aspects of Galaxy Dynamics Using Planetary Nebulae" @default.
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- W201306114 doi "https://doi.org/10.1017/s0074180900209868" @default.
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