Radial-velocity measurements of the lunar-occultation binaries 66 Ari and HD 64704

Details Radial-velocity measurements of the lunar-occultation binaries 66 Ari and HD 64704 Radial-velocity measurements of the lunar-occultation binaries 66 Ari and HD 64704

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984obs...104...69g&link_type=abstract

The Observatory, vol. 104, p. 69-74 (1984)

Physics

6

Scientific paper

66 Ari A, which was found by the occultation method to be double with a projected linear separation of only about 1/2 AU, has for ten years maintained a constant radial velocity which is the same as it had in 1920. The most likely explanation is that it is not in fact double. HD 64704, whose duplicity has been confirmed by direct observation, shows marginal radial-velocity changes on a time-scale commensurate with that of the visual orbit.

Affiliated with

Also associated with

No associations

Rating

Radial-velocity measurements of the lunar-occultation binaries 66 Ari and HD 64704 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 Radial-velocity measurements of the lunar-occultation binaries 66 Ari and HD 64704, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radial-velocity measurements of the lunar-occultation binaries 66 Ari and HD 64704 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1500785