Milky Way rotation and the distance to the Galactic center from Cepheid variables
Milky Way rotation and the distance to the Galactic center from Cepheid variables
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DOI:
10.1007/3-540-19484-3_8
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发表时间:
1987-05
期刊:
影响因子:
--
通讯作者:
J. Caldwell;I. Coulson
中科院分区:
文献类型:
--
作者:
J. Caldwell;I. Coulson
The existing data on Milky Way Cepheids are fitted with an axisymmetric Galactic rotation model. A new “standard candle” mois determined: the unreddened apparent magnitude of a hypothetical Cepheid with standard period, color, and metallicity at a distance of 1 Ro. It then follows that Ro = 7.8 ± 0.7 kpc from the cluster Cepheid zero point. Further important results are that 2AR0= 228 ± 19 km s−1, and that the observed Cepheid mean velocities average 3.1 ± 0.9 km s−1too negative compared with the center-of-mass velocities.