We report on the determination of the visual orbit of the double-lined spectroscopic binary system 12 Bootis with data obtained by the Palomar Testbed Interferometer in 1998 and 1999. 12 Boo is a nearly equal-mass double-lined binary system whose spectroscopic orbit is well known. We have estimated the visual orbit of 12 Boo from our interferometric visibility data Ðtted both separately and in conjunction with archival and CORAVEL radial velocity data. Our 12 Boo orbit is in good agreement with the spectroscopic results, and the physical parameters implied by a combined Ðt to our visibility data and radial velocity data result in precise component masses. In particular, the orbital parallax of the system is determined to be 27.09 ^ 0.41 mas...
Radial-velocity measurements and sine-curve fits to orbital radial velocity variations are presented...
We have determined the visual orbit for the spectroscopic binary L Pegasi with interferometric visib...
We present an updated spectroscopic orbit and a new visual orbit for the double-lined spectroscopic ...
In a previous paper we reported on the binary system 12Bootis and its evolutionary state. In particu...
We report on a significantly improved determination of the physical orbit of the double-lined spectr...
We report on the determination of the visual orbit of the double-lined spectroscopic binary system 6...
Radial velocities from the 2.1 m telescope at McDonald Observatory supplemented with radial velociti...
Contains fulltext : 32820.pdf (publisher's version ) (Open Access)The bright south...
Vita.An astrometric study of E-Bootis (a=14(superscript h)46(superscript m).8, δ=19°31',1900) also k...
We report on the determination of the visual orbit of the double-lined spectroscopic binary system 6...
In this paper the preliminary orbital elements are presented for the following double stars: WDS 001...
WOS: 000305375200002In this study, we present the first Johnson BV photometry of the eclipsing binar...
Differential astrometry measurements from the Palomar High-precision Astrometric Search for Exoplane...
Spectra taken at Bosque Alegre from 1949 through 1951 and from 1960 through 1963 have confirmed that...
Evolutionary tracks are of key importance for the understanding of star formation. Unfortunately, tr...
Radial-velocity measurements and sine-curve fits to orbital radial velocity variations are presented...
We have determined the visual orbit for the spectroscopic binary L Pegasi with interferometric visib...
We present an updated spectroscopic orbit and a new visual orbit for the double-lined spectroscopic ...
In a previous paper we reported on the binary system 12Bootis and its evolutionary state. In particu...
We report on a significantly improved determination of the physical orbit of the double-lined spectr...
We report on the determination of the visual orbit of the double-lined spectroscopic binary system 6...
Radial velocities from the 2.1 m telescope at McDonald Observatory supplemented with radial velociti...
Contains fulltext : 32820.pdf (publisher's version ) (Open Access)The bright south...
Vita.An astrometric study of E-Bootis (a=14(superscript h)46(superscript m).8, δ=19°31',1900) also k...
We report on the determination of the visual orbit of the double-lined spectroscopic binary system 6...
In this paper the preliminary orbital elements are presented for the following double stars: WDS 001...
WOS: 000305375200002In this study, we present the first Johnson BV photometry of the eclipsing binar...
Differential astrometry measurements from the Palomar High-precision Astrometric Search for Exoplane...
Spectra taken at Bosque Alegre from 1949 through 1951 and from 1960 through 1963 have confirmed that...
Evolutionary tracks are of key importance for the understanding of star formation. Unfortunately, tr...
Radial-velocity measurements and sine-curve fits to orbital radial velocity variations are presented...
We have determined the visual orbit for the spectroscopic binary L Pegasi with interferometric visib...
We present an updated spectroscopic orbit and a new visual orbit for the double-lined spectroscopic ...