J/AJ/160/141         Astrometric measurements of * bet LMi         (Wang+, 2020)

The improved orbit solution and component masses of bet LMi. Wang X., Xia F., Fu Y. <Astron. J., 160, 141 (2020)> =2020AJ....160..141W 2020AJ....160..141W
ADC_Keywords: Stars, double and multiple; Positional data Keywords: Binary stars ; Fundamental parameters of stars ; Visual binary stars ; Spectroscopic binary stars Abstract: bet LMi is a double-lined visual binary with an orbital period of ∼39yr. Via a simultaneous fitting to both astrometric and radial velocity measurements, we give a complete and improved orbit solution with high precision. Then, the component masses are precisely determined as 2.98±0.10M☉ and 1.92±0.04M☉ with a relative precision of ∼3%, respectively. The orbital parallax is determined to be 19.6±0.2mas, which is two times more precise than Hipparcos parallax. With the known apparent magnitudes and magnitude difference of the components, we derive the luminosity of the components as 50.7±1.8L☉ and 9.1±4.1L☉. The estimated radii of the components are 9.4±0.3R☉ and 3.7±1.5R☉. Description: We extract the relative astrometric measurements of the two components from the Fourth Catalog of Interferometric Measurements of Binary Stars (Hartkopf+, 2001). Objects: ----------------------------------------------- RA (2000) DE Designation(s) ----------------------------------------------- 10 27 53.00 +36 42 26.0 * bet LMi = HD 90537 ----------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 61 80 The relative astrometric measurements, adopted errors and residuals in the rectangular coordinates -------------------------------------------------------------------------------- See also: I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007) J/AJ/106/1639 : Speckle observations of binary stars (McAlister+ 1993) J/A+AS/105/503 : Binary star speckle measurements (Balega+ 1994) J/AJ/108/2299 : ICCD speckle obs. of binary stars. XI. (Hartkopf+, 1994) J/ApJ/469/355 : Teff, B-V and BC relation (Flower, 1996) J/A+A/341/121 : Visual binary orbits and masses (Soederhjelm 1999) J/A+AS/141/371 : Low-mass stars evolut. tracks & isochrones (Girardi+,2000) J/AJ/119/3084 : ICCD speckle obs. of binary stars. XXIII. (Hartkopf+, 2000) J/AJ/119/1448 : Improved properties for cool stars (Houdashelt+, 2000) J/AJ/127/1727 : Differential magnitudes of binary stars (Horch+, 2004) J/AJ/135/209 : Rotational and RVs 761 HIP giants (Massarotti+, 2008) J/MNRAS/395/907 : PISCO speckle observations in 2007 (Prieur+, 2009) J/AJ/140/1579 : PHASES differential astrometry data (Muterspaugh+, 2010) J/AJ/142/176 : Exoplanet host stars.II. Speckle interferometry (Mason+,2011) J/AJ/149/110 : Radial velocities of 47 Oph (Wang+, 2015) J/ApJ/817/40 : High-resolution NIR spectra of local giants (Feuillet+, 2016) J/A+A/585/A73 : PTPS stars. III. The evolved stars sample (Niedzielski+,2016) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 F9.4 yr Epoch [1935/2013] Besselian year of the epoch of observation 11- 18 F8.5 arcsec x [-0.43/0.1] x position offset 20- 26 F7.5 arcsec e_x [0.001/0.05] Uncertainty in x 28- 35 F8.5 arcsec (O-C)x [-0.06/0.06] Residual in x 37- 44 F8.5 arcsec y [-0.44/0.09] y position offset 46- 52 F7.5 arcsec e_y [0.002/0.06] Uncertainty in y 54- 61 F8.5 arcsec (O-C)y [-0.06/0.05] Residual in y -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Coralie Fix [CDS], 13-Nov-2020
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