Common proper motions stars in AGK3

The 326 common proper motion systems that have a ratio angular separation to proper motion smaller than 1000 years are in table1. The number of optical systems is expected to be around 4. Each system fills a 256 byte-length record that may also be considered as two 128 byte-length records for print-out edition. The 113 common proper motion systems that have a ratio angular separation to proper motion between 1000 and 3500 years are in table2. The number of physical systems is expected to be around 68. The presentation is the same as for table1. This table differs from the original printed version, since the the magnitude and the spectral type of the secondary component of the 47th system were corrected. The system 47 was also added to the notes.

Cone search capability for table I/121/cpm (Combined table from original tables)

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/I/121
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/I/121
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=I/121
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/I/121
Provenance
Creator Halbwachs J.L.
Publisher CDS
Publication Year 2013
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Galactic and extragalactic Astronomy; Natural Sciences; Physics; Stellar Astronomy