The triple system ADS 9167 (Kiyaeva+, 1998)

Details The triple system ADS 9167 (Kiyaeva+, 1998) The triple system ADS 9167 (Kiyaeva+, 1998)

Feb 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ycat..90240868k&link_type=abstract

VizieR On-line Data Catalog: J/PAZh/24/868. Originally published in: 1998PAZh...24..868K; 1998AstL...24..753K

Computer Science

Binaries: Spectroscopic, Stars: Double And Multiple, Radial Velocities

Scientific paper

It is found from the observations with the correlation radial velocity meter that the primary component of the visual double star ADS 9167 is a single-lined spectroscopic binary with 2.87- yr period and 0.75 eccentricity. Using the 26-year-long series of Pulkovo photographic relative-positions observations, a new visual orbit of AB is calculated with a period of about 1000 years. (2 data files).

Affiliated with

Also associated with

No associations

Rating

The triple system ADS 9167 (Kiyaeva+, 1998) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The triple system ADS 9167 (Kiyaeva+, 1998), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The triple system ADS 9167 (Kiyaeva+, 1998) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-950682