J/AJ/162/260     Mass ratios of 248 long-period binary stars    (Makarov+, 2021)

Astrometric mass ratios of 248 long-period binary stars resolved in Hipparcos and Gaia EDR3. Makarov V.V., Fabricius C. <Astron. J., 162, 260-260 (2021)> =2021AJ....162..260M 2021AJ....162..260M (SIMBAD/NED BibCode)
ADC_Keywords: Stars, double and multiple; Stars, masses; Optical; Parallaxes, trigonometric; Positional data Keywords: Mass ratio; Astrometric binary stars; Optical double stars; Astrometry Abstract: Using the absolute astrometric positions and proper motions for common stars in the Hipparcos and Gaia catalogs separated by 24.75yr in the mean epoch, we compute mass ratios for long-period, resolved binary systems without any astrophysical assumptions or dependencies, except the presence of inner binary subsystems that may perturb the observed mean proper motions. The mean epoch positions of binary companions from the Hipparcos Double and Multiple System Annex are used as the first epoch. The mean positions and proper motions of carefully cross-matched counterparts in Gaia EDR3 comprise the second epoch data. Selecting only results with sufficiently high signal-to-noise ratio and discarding numerous optical pairs, we construct a catalog of 248 binary systems, which is published online. Several cases with unusual properties or results are also discussed. Description: Using commonly accessible information from the ESA's Hipparcos and Gaia space missions, we were able to process the entire cross-matched sample of resolved double stars and selected 248 high-probability binary systems with statistically significant estimates of mass ratio. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 363 248 Star catalog of resolved binaries with astrometric mass ratios from Hipparcos & Gaia -------------------------------------------------------------------------------- See also: I/239 : The Hipparcos and Tycho Catalogues (ESA 1997) I/276 : Tycho Double Star Catalogue (TDSC) (Fabricius+ 2002) I/337 : Gaia DR1 (Gaia Collaboration, 2016) I/350 : Gaia EDR3 (Gaia Collaboration, 2020) J/ApJS/224/19 : The KepVIM catalog (Makarov+, 2016) J/MNRAS/471/770 : Parameters & IR excesses of Gaia DR1 stars (McDonald+, 2017) J/AJ/157/136 : RVs of RGs with suspected massive companions (Makarov+, 2019) J/AJ/160/268 : Infrared photometry of binaries in Orion OB1 (Tokovinin+, 2020) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- PHip Primary Hipparcos identifier 8 A1 --- PHipCom Primary Hipparcos component identifier 10- 15 I6 --- SHip Secondary Hipparcos identifier 17 A1 --- SHipCom Secondary Hipparcos component identifier 19- 37 I19 --- Gaia Primary Gaia EDR3 identifier 39- 50 F12.8 deg RAdeg [1/360] Primary Gaia EDR3 Right Ascension (J2016) 52- 63 F12.8 deg DEdeg [-85/76] Primary Gaia EDR3 Declination (J2016) 65- 71 F7.3 mas plx [3.32/284] Primary Gaia EDR3 parallax 73- 81 F9.3 mas/yr pmRA [-1312/1749] Primary Gaia EDR3 proper motion along RA 83- 91 F9.3 mas/yr pmDE [-1163/1793] Primary Gaia EDR3 proper motion along DE 93- 97 F5.3 arcsec e_RAdeg [0.009/0.6] Uncertainty in PRAdeg 99-103 F5.3 arcsec e_DEdeg [0.008/0.7] Uncertainty in PDEdeg 105-109 F5.3 mas e_plx [0.01/0.8] Uncertainty in Pplx 111-115 F5.3 mas/yr e_pmRA [0.009/0.7] Uncertainty in PpmRA 117-121 F5.3 mas/yr e_pmDE [0.01/0.9] Uncertainty in PpmDE 123-132 F10.3 --- chi2 [298/789599] Primary astrometric χ2 134-139 F6.3 --- RUWE [0.66/18.7] Primary RUWE parameter 141-146 F6.3 mag Gmag [3.32/11.7] Primary Gaia EDR3 G band apparent magnitude 148-153 F6.3 mag Gbpmag [3.09/12.4] Primary Gaia EDR3 Blue passband apparent magnitude 155-160 F6.3 mag Grpmag [2.84/10.2] Primary Gaia EDR3 Red passband apparent magnitude 162-180 I19 --- Gaia2 Secondary Gaia EDR3 identifier 182-193 F12.8 deg RAdeg2 [1/360] Secondary Gaia EDR3 Right Ascension (J2016) 195-206 F12.8 deg DEdeg2 [-85/76] Secondary Gaia EDR3 Declination (J2016) 208-214 F7.3 mas plx2 [3.97/284] Secondary Gaia EDR3 parallax 216-224 F9.3 mas/yr pmRA2 [-1401/1704] Secondar Gaia EDR3 proper motion along RA 226-234 F9.3 mas/yr pmDE2 [-1167/1863] Secondar Gaia EDR3 proper motion along DE 236-240 F5.3 mas e_RAdeg2 [0.008/0.5] Uncertainty in SRAdeg 242-246 F5.3 mas e_DEdeg2 [0.009/0.6] Uncertainty in SDEdeg 248-252 F5.3 mas e_plx2 [0.01/0.8] Uncertainty in Splx 254-258 F5.3 mas/yr e_pmRA2 [0.009/0.7] Uncertainty in SpmRA 260-264 F5.3 mas/yr e_pmDE2 [0.01/0.8] Uncertainty in SpmDE 266-275 F10.3 --- chi22 [263/179164] Secondary astrometric χ2 277-282 F6.3 --- RUWE2 [0.69/18.8] Secondary RUWE parameter 284-290 F7.3 mag Gmag2 [3.98/12.1]? Secondary Gaia EDR3 G band apparent magnitude 292-298 F7.3 mag Gbpmag2 [3.32/12.8]? Secondary Gaia EDR3 Blue passband apparent magnitude 300-306 F7.3 mag Grpmag2 [3.4/10.3]? Secondary Gaia EDR3 Red passband apparent magnitude 308-312 F5.3 --- q [0.02/9.13] Ratio; secondary/primary masses 314-317 F4.1 deg eta [0/49.5] Alignment angle 319-323 F5.3 --- e_q [0.005/3] Lower bound error in q 325-329 F5.3 --- E_q [0.005/3] Upper bound error in q 331-335 F5.3 --- qmean [0.02/8.37] Median q from MC simulations 337-345 F9.3 --- SNR [10.8/53133] Signal-to-Noise ratio 347-355 F9.3 mas Sep [408/13327] Gaia EDR3 separation (J2016) 357-361 F5.1 deg PA [1.1/360] Gaia EDR3 position angle (J2016) 363 I1 --- Q [1/3] Quality flag (1) -------------------------------------------------------------------------------- Note (1): The highest quality solutions (flag 1) are those with SNR>50 and η<7.45deg, the lowest quality (flag 3) is assigned to entries with SNR<50 and η>7.45deg, and the quality 2 comprises the remaining solutions. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Coralie Fix [CDS], 22-Feb-2022
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line