Other
Scientific paper
Feb 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aj....129.1001f&link_type=abstract
The Astronomical Journal, Volume 129, Issue 2, pp. 1001-1007.
Other
8
Stars: Binaries: Spectroscopic, Stars: Fundamental Parameters, Stars: Variables: Other
Scientific paper
We have obtained extensive spectroscopic and velocity spectrometer observations of HD 166181, a previously known single-lined spectroscopic binary. Our improved orbit for the G6 V primary has a period of 1.8098343 days and is circular. Although the lines of additional components have not been detected, radial velocity measurements confirm that the system has additional velocity variations with a period of 2092 days, or 5.73 yr. This long-period orbit has an eccentricity of 0.76. An analysis of the Hipparcos observations produces a well-determined astrometric orbit for the long-period system that has an inclination of 78°. Mass estimates of the components in this zero-age main-sequence multiple system indicate that the unseen secondary in the 5.73 yr orbit may also be a binary. Thus, HD 166181 is at least a triple system and possibly quadruple.
Barlow D. J.
Fekel Francis C.
Jancart Sylvie
Pourbaix Dimitri
Scarfe Colin D.
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