Velocity standards that have variable velocities. I - HD 184467

Details Velocity standards that have variable velocities. I - HD 184467 Velocity standards that have variable velocities. I - HD 184467

Mar 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983pasp...95..201m&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 95, March 1983, p. 201-205.

Astronomy and Astrophysics

Astronomy

15

Astronomical Spectroscopy, Binary Stars, Orbital Elements, Radial Velocity, Reference Stars, Ephemerides, Orbit Calculation, Spectrometers

Scientific paper

In connection with observations conducted with a photoelectric radial-velocity spectrometer (RVS) on a 1.2-m telescope, several variable-velocity stars have been discovered among lists of standard-velocity stars. HD 184467 is a 7.4 B magnitude K1 V star from Table II of the IAU list. On the basis of the RVS observations, it was found that this star is a double-line binary. The maximum separation in the velocities of the two components is only 28 km/s, and the double-line phase occurs less than 20 percent of the time even at coudedispersions. A description is provided of the observations and orbit of HD 184467.

Affiliated with

Also associated with

No associations

Rating

Velocity standards that have variable velocities. I - HD 184467 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 Velocity standards that have variable velocities. I - HD 184467, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Velocity standards that have variable velocities. I - HD 184467 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1470388