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A&A 367, 967-972 (2001)
DOI: 10.1051/0004-6361:20000439
The distances of planetary nebulae: A scaling factor based upon radial velocities
J. P. PhillipsInstituto de Astronomia y Meteorologia, Avenida Vallarta 2602, Col. Arcos Vallarta, CP 44130 Guadalajara, Jalisco, Mexico
(Received 19 May 2000 /Accepted 1 December 2000 )
Abstract
We have used the observed radial velocities of planetary nebulae,
and the galactic rotation curve to define a new distance scale
for planetary nebulae. Care has been taken to restrict the
analysis to sources in which distance non-linearities are
minimised, and for which distortion of the distance scale is
likely to be small. We conclude, as a result, that the so-called
"long"distance scales are the most valid, and that various
"shorter"scales are unlikely to be correct. The primary
systematic errors in this procedure derive from uncertainties in
the galactic rotation profile, and in
and R0. Such errors are less than those normally associated
with PN distance determinations.
Key words: planetary nebulae: general -- Galaxy: kinematics and dynamics
Offprint request: J. P. Phillips, jpp@udgserv.cencar.udg.mx
SIMBAD Objects in preparation
© ESO 2001
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