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Solar Motion‐ and Galactic Rotation‐Terms from AGK 3 Proper Motions
Author(s) -
Dieckvoss W.
Publication year - 1967
Publication title -
astronomische nachrichten
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.394
H-Index - 63
eISSN - 1521-3994
pISSN - 0004-6337
DOI - 10.1002/asna.19672900402
Subject(s) - physics , differential rotation , astrophysics , rotation (mathematics) , proper motion , stars , motion (physics) , astronomy , magnitude (astronomy) , classical mechanics , geometry , mathematics
In three tables results of a statistical study from 163811 stars grouped according to spectral type and apparent magnitude are presented for apex of solar motion, secular parallaxes, linear terms of differential galactic rotation. The latter are lying closely to the recommended preliminary values of + 15, ‐10 km/s/kpc.