The following document lists the file notes.dat
from catalogue J/A+A/430/165.
Also available:
plain copy of the file
with f77 program to read file
into arrays
or line by line
File is also available in
FITS,
Tab-separated format,
or in HTML.
## (from tabmap V6.0 (2016-08-18)) 2024-05-19T15:14:14 #--------------------------------------------------------------------------- #-- J/A+A/430/165 Radial velocities for 6691 K and M giants (Famaey+, 2005) #-------------------------------------------------------------------------- #---Table: J/A+A/430/165/./notes.dat Individual notes (19 records) # HIP I6 --- HIP number # Note A73 --- Text of Note -------------------------------------------------------------------------------- HIP|Note ------|------------------------------------------------------------------------- 779|Very distant star (first-order correction to the differential galactic 779| rotation inaccurate); binary of VV Cep type (M1epIb + B2.6V) 1050|Tyc 8-743-1 = BD +04 19 different from HIC 1050; hence V-I H40 is wrong 7351|Tyc 4301 1334 1 and 4301 2069 1: common proper motion pair 12416|Very distant star (first-order correction to the differential galactic 12416| rotation inaccurate) 24417|Tyc 4347 1772 1 and 4347 1769 1: common proper motion pair 29425|Binary of VV Cep type (M2epIab+B2-3V) 30997|A visual binary with a separation of 4.2" (magnitudes V~9.1 and 9.4). 30997|The presence of this companion confused the Hipparcos solution, which is 30997|totally unreliable. This star was not used in the kinematic analysis. 34484|The two visual components have similar radial velocities 52223|The two visual components have similar radial velocities 64411|The two visual components have similar radial velocities 108317|Binary of VV Cep type (M2epIa-Iab+B8:eV) 111592|Very distant star (first-order correction to the differential galactic 111592| rotation inaccurate); binary of VV Cep type (K0ep-M2epIa+B0/B1) 117078|Very distant star (first-order correction to the differential galactic 117078| rotation inaccurate) --------------------------------------------------------------------------------