J/AJ/132/1910  HD 131861 radial velocities and VRI light curves (Fekel+, 2006)

HD 131861, a double-line spectroscopic triple system. Fekel F.C., Henry G.W., Barlow D.J., Pourbaix D. <Astron. J., 132, 1910-1917 (2006)> =2006AJ....132.1910F 2006AJ....132.1910F
ADC_Keywords: Stars, double and multiple ; Radial velocities ; Photometry, VRI Keywords: binaries: eclipsing - binaries: spectroscopic - stars: fundamental parameters Abstract: Our red-wavelength spectroscopic observations of HD 131861, a previously known single-line multiple system, span 20 years. Now lines of two components, the short-period F5 V primary and G8 V secondary, have been detected. The inner orbit is circular with a period of 3.5507439-days, while the outer orbit of the system has a period of 1642 days or 4.496-yr and a relatively low eccentricity of 0.10. Analysis of the Hipparcos data produces a well-determined astrometric orbit for the long-period system that has an inclination of 52°. Our photometric observations show shallow primary and secondary eclipses of the short-period pair, and eclipse solutions result in an inclination of 81°. Thus, the long- and short-period orbits are not coplanar. The mass of the unseen third component is 0.7M{dot}, corresponding to a mid-K dwarf. The total mass of the system, 3.08M{dot}, leads to a semimajor axis of 4AU for the outer orbit. The F5 V primary is rotating more slowly than it would if it were synchronously rotating, while the G8 V secondary may be synchronously rotating. The lithium abundance of the F5 V primary is similar to the initial lithium abundance found for Population I dwarfs and so indicates no significant dilution. Description: From 1984 March through 2005 June we obtained 64 spectrograms of HD 131861 at the Kitt Peak National Observatory (KPNO) with the coude feed telescope, coude spectrograph, and a Texas Instruments CCD detector. The first seven observations, obtained from 1984 through 1987, used grating D, which resulted in a wavelength range of about 90Å and a resolution of 0.23Å. One spectrogram was centered at 6700Å, while all the rest were obtained at 6430Å. From 1988 onward grating A was used, which produced spectrograms with a wavelength range of over 80Å and a resolution of 0.21Å. The vast majority of the grating A observations were centered at 6430Å, while four were obtained at 6700Å. Objects: ------------------------------------------------------------------ RA (2000) DE Designation(s) (star) ------------------------------------------------------------------ 14 54 24.5 +45 17 55.7 HD 131861 = HIP 72939 (variable) 14 44 28.2 +45 11 09.6 HD 130044 = HIP 72066 (comparison) 14 49 18.7 +46 06 58.4 HD 130945 = HIP 72487 (check) ------------------------------------------------------------------ File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 53 87 Radial velocities of HD 131861 table2.dat 54 2113 Photometric observations of HD 131861 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 F11.3 d HJD Heliocentric Julian date 12 A1 --- n_HJD [b] b: Lithium region (λ=6700Å) 14- 18 F5.3 --- phiL [0/1] Phase in the long-period orbit 20- 24 F5.3 --- phiS ]0/1[ Phase in the short-period orbit 26- 30 F5.1 km/s RVAa Aa component radial velocity 32- 35 F4.1 km/s (O-C)Aa Aa component observed minus Computer radial velocity 37- 42 F6.1 km/s RVAb ?=- Ab component radial velocity 43 A1 --- n_RVAb [a] a: 3σ residual, velocity given zero weight. 44- 47 F4.1 km/s (O-C)Ab ?=- Ab component Observed minus Computer radial velocity 50- 53 A4 --- Obs Onservatory (HPO or KPNO) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 F12.4 --- HJD Heliocentric Julian Date 14- 19 F6.3 mag DV(V-C) ?=99.999 Var-Comp differential V magnitude (1) 21- 26 F6.3 mag DR(V-C) ?=99.999 Var-Comp differential R magnitude (1) 28- 33 F6.3 mag DI(V-C) ?=99.999 Var-Comp differential I magnitude (1) 35- 40 F6.3 mag DV(Ck-C) ?=99.999 Check-Comp differential V magnitude (1) 42- 47 F6.3 mag DR(Ck-C) ?=99.999 Check-Comp differential R magnitude (1) 49- 54 F6.3 mag DI(Ck-C) ?=99.999 Check-Comp differential I magnitude (1) -------------------------------------------------------------------------------- Note (1): The '99.999' signifies that the differential magnitude was discarded because its internal standard deviation exceeded 0.02mag. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Vannier [CDS] 24-Jul-2008
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