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- W2105602005 abstract "The galactic rotation curve is determined on the basis of a large sample of planetary nebulae with known radial velocities. Four distance scales are adopted and the curve is established for galactocentric distances of 4 to 14 kpc, approximately, adopting R0 = 8:5 kpc for the galactocentric distance of the LSR. The main conclusions are: (i) there is no indication of a measurable decrease of the rotation curve beyond the solar circle; (ii) there are no important dierences among the statistical distance scales considered, irrespective of the short or long nature of the scale, even though individual nebulae can have very dieren t distances according to the dieren t scales, and (iii) the derived curves are similar to the rotation curve derived from H II regions, taking into account the fact that PN are generally older objects and have larger velocity components perpendicular to the galactic plane." @default.
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- W2105602005 date "2005-10-01" @default.
- W2105602005 modified "2023-09-23" @default.
- W2105602005 title "A NEW DETERMINATION OF THE ROTATION CURVE FROM GALACTIC DISK PLANETARY NEBULAE" @default.
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