The three-body system V 505 Sagittarii.

Details The three-body system V 505 Sagittarii. The three-body system V 505 Sagittarii.

Aug 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26a...324..988m&link_type=abstract

Astronomy and Astrophysics, v.324, p.988-990

Astronomy and Astrophysics

Astrophysics

14

Binaries: Eclipsing, Binaries: Visual, Stars: Individual: V 505 Sgr

Scientific paper

It is known that the period of the eclipsing binary V 505 Sgr changes, and that the changes can be explained - at least partly - by a light-time effect. The system is also known as a speckle binary. In this paper parameters of the third body orbit are suggested in order to explain both sets of data. Some discrepancies in the size of the orbit and radial velocity data remain. Next periastron passage should be at 1998.9.

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