Gaia Data Release 3 Stellar multiplicity, a teaser for the hidden treasure

被引:118
作者
Arenou, F. [1 ]
Babusiaux, C. [1 ,2 ]
Barstow, M. A. [3 ]
Faigler, S. [4 ]
Jorissen, A. [5 ]
Kervella, P. [6 ]
Mazeh, T. [4 ]
Mowlavi, N. [7 ]
Panuzzo, P. [1 ]
Sahlmann, J. [8 ]
Shahaf, S. [9 ]
Sozzetti, A. [10 ]
Bauchet, N. [1 ]
Damerdji, Y. [11 ,12 ]
Gavras, P. [8 ]
Giacobbe, P. [10 ]
Gosset, E. [11 ,13 ]
Halbwachs, J. -L. [14 ]
Holl, B. [7 ,15 ]
Lattanzi, M. G. [10 ,16 ]
Leclerc, N. [1 ]
Morel, T. [11 ]
Pourbaix, D. [5 ,13 ]
Re Fiorentin, P. [10 ]
Sadowski, G. [5 ]
Segransan, D. [7 ]
Siopis, C. [5 ]
Teyssier, D. [17 ]
Zwitter, T. [18 ]
Planquart, L. [5 ]
Brown, A. G. A. [19 ]
Vallenari, A. [20 ]
Prusti, T. [21 ]
de Bruijne, J. H. J. [21 ]
Biermann, M. [22 ]
Creevey, O. L. [23 ]
Ducourant, C. [24 ]
Evans, D. W. [25 ]
Eyer, L. [7 ]
Guerra, R. [26 ]
Hutton, A. [27 ]
Jordi, C. [28 ]
Klioner, S. A. [29 ]
Lammers, U. L. [26 ]
Lindegren, L. [30 ]
Luri, X. [28 ]
Mignard, F. [23 ]
Panem, C. [31 ]
Randich, S. [32 ]
Sartoretti, P. [1 ]
机构
[1] Univ PSL, GEPI, CNRS, Observ Paris, 5 Pl Jules Janssen, F-92190 Meudon, France
[2] Univ Grenoble Alpes, CNRS, IPAG, F-38000 Grenoble, France
[3] Univ Leicester, Sch Phys & Astron, Space Pk Leicester,Univ Rd, Leicester LE1 7RH, Leics, England
[4] Tel Aviv Univ, Sch Phys & Astron, IL-6997801 Tel Aviv, Israel
[5] Univ Libre Bruxelles, Inst Astron & Astrophys, CP 226,Blvd Triomphe, B-1050 Brussels, Belgium
[6] Univ Paris, Sorbonne Univ, CNRS, LESIA,Observ Paris,Univ PSL, 5 Pl Jules Janssen, F-92190 Meudon, France
[7] Univ Geneva, Dept Astron, Chemin Pegasi 51, CH-1290 Versoix, Switzerland
[8] European Space Agcy, RHEA, Camino Bajo Castillo S-N, Madrid 28692, Spain
[9] Weizmann Inst Sci, Dept Particle Phys & Astrophys, IL-7610001 Rehovot, Israel
[10] Osserv Astron Torino, INAF, Via Osservatorio 20, I-10025 Pino Torinese, TO, Italy
[11] Univ Liege, Inst Astrophys & Geophys, 19c Allee 6 Aout, B-4000 Liege, Belgium
[12] Ctr Rech Astron Astrophys & Geophys, Route Observ Bp 63 Bouzareah, Algiers 16340, Algeria
[13] FRS FNRS, Rue Egmont 5, B-1000 Brussels, Belgium
[14] Univ Strasbourg, CNRS, UMR 7550, Observ Astron Strasbourg, 11 Rue Univ, F-67000 Strasbourg, France
[15] Univ Geneva, Dept Astron, Chemin Ecogia 16, CH-1290 Versoix, Switzerland
[16] Univ Turin, Dept Phys, Via Pietro Giuria 1, I-10125 Turin, Italy
[17] European Space Agcy, Telespazio UK SL, Camino Bajo Castillo S-N, Madrid 28692, Spain
[18] Univ Ljubljana, Fac Math & Phys, Jadranska Ulica 19, Ljubljana 1000, Slovenia
[19] Leiden Univ, Leiden Observ, Niels Bohrweg 2, NL-2333 CA Leiden, Netherlands
[20] Osserv Astron Padova, INAF, Vicolo Osservatorio 5, I-35122 Padua, Italy
[21] European Space Agcy, European Space Res & Technol Ctr, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands
[22] Heidelberg Univ, Astron Rech Inst, Zentrum Astron, Monchhofstr 12-14, D-69120 Heidelberg, Germany
[23] Univ Cote Azur, Observ Cote Azur, CNRS, Lab Lagrange, Bd Observ,CS 34229, F-06304 Nice 4, France
[24] Univ Bordeaux, CNRS, Lab Astrophys Bordeaux, B18N,Allee Geoffroy St Hilaire, F-33615 Pessac, France
[25] Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England
[26] European Space Agcy, European Space Technol Ctr, Camino Bajo Castillo S-N, Madrid 28692, Spain
[27] European Space Agcy, Aurora Technol, Camino Bajo Castillo S-N, Madrid 28692, Spain
[28] Univ Barcelona IEEC UB, Inst Ciencies Cosmos ICCUB, Marti & Franques 1, Barcelona 08028, Spain
[29] Tech Univ Dresden, Lohrmann Observ, Mommsenstr 13, D-01062 Dresden, Germany
[30] Lund Univ, Lund Observ, Dept Astron & Theoret Phys, Box 43, S-22100 Lund, Sweden
[31] CNES Ctr Spatial Toulouse, 18 Ave Edouard Belin, F-31401 Toulouse 9, France
[32] Osserv Astrofis Arcetri, INAF, Largo Enrico Fermi 5, I-50125 Florence, Italy
[33] Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany
[34] European Space Agcy, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands
[35] Osservatorio Astrofis & Sci Spazio Bologna, INAF, Via Piero Gobetti 93-3, I-40129 Bologna, Italy
[36] Univ Barcelona IEEC UB, Inst Ciencies Cosmos ICCUB, DAPCOM, Marti & Franques 1, Barcelona 08028, Spain
[37] Royal Observ Belgium, Ringlaan 3, B-1180 Brussels, Belgium
[38] Uppsala Univ, Observat Astrophys, Div Astron & Space Phys, Dept Phys & Astron, Box 516, S-75120 Uppsala, Sweden
[39] ALTEC Spa, Corso Marche 79, I-10146 Turin, Italy
[40] Sednai Sarl, Geneva, Switzerland
[41] Univ Coll London, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England
[42] ESAC, Gaia DPAC Project Off, Camino Bajo Castillo S-N, Madrid 28692, Spain
[43] Sorbonne Univ, Univ PSL, Observ Paris, SYRTE,CNRS,LNE, 61 Ave Observ, F-75014 Paris, France
[44] Natl Observ Athens, Athens 15236, Greece
[45] Univ Lille, Sorbonne Univ, CNRS, IMCCE,Observ Paris,Univ PSL, 77 Ave Denfert Rochereau, F-75014 Paris, France
[46] European Space Agcy, Serco Gest Negocios, Camino Bajo Castillo S-N, Madrid 28692, Spain
[47] Univ Edinburgh, Inst Astron, Royal Observ, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland
[48] European Space Agcy, ATG Europe, Camino Bajo Castillo S-N, Madrid 28692, Spain
[49] Univ A Coruna, CIGUS CITIC Dept Comp Sci & Informat Technol, Campus Elvina S-N, La Coruna 15071, Spain
[50] Kavli Inst Cosmol Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England
基金
欧洲研究理事会; 比利时弗兰德研究基金会;
关键词
binaries; general; astrometry; planetary systems; stars; fundamental parameters; catalogs; white dwarfs; EXTRA-SOLAR PLANETS; HUBBLE-SPACE-TELESCOPE; BROWN DWARF DESERT; INDIVIDUAL DYNAMICAL MASSES; 1ST SPECTROSCOPIC DATA; DIGITAL SKY SURVEY; 6TH DATA RELEASE; ECLIPSING-BINARY; WHITE-DWARFS; BLACK-HOLE;
D O I
10.1051/0004-6361/202243782
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Context. The Gaia DR3 catalogue contains, for the first time, about 800 000 solutions with either orbital elements or trend parameters for astrometric, spectroscopic, and eclipsing binaries, and combinations of these three.Aims. With this paper, we aim to illustrate the huge potential of this large non-single-star catalogue.Methods. Using the orbital solutions and models of the binaries, we have built a catalogue of tens of thousands of stellar masses or lower limits thereof, some with consistent flux ratios. Properties concerning the completeness of the binary catalogues are discussed, statistical features of the orbital elements are explained, and a comparison with other catalogues is performed.Results. Illustrative applications are proposed for binaries across the Hertzsprung-Russell Diagram (HRD). Binarity is studied in the giant branch and a search for genuine spectroscopic binaries among long-period variables is performed. The discovery of new EL CVn systems illustrates the potential of combining variability and binarity catalogues. Potential compact object companions are presented, mainly white dwarf companions or double degenerates, but one candidate neutron star is also found. Towards the bottom of the main sequence, the orbits of previously suspected binary ultracool dwarfs are determined and new candidate binaries are discovered. The long awaited contribution of Gaia to the analysis of the substellar regime shows the brown dwarf desert around solar-type stars using true rather than minimum masses, and provides new important constraints on the occurrence rates of substellar companions to M dwarfs. Several dozen new exoplanets are proposed, including two with validated orbital solutions and one super-Jupiter orbiting a white dwarf, all being candidates requiring confirmation. Besides binarity, higher order multiple systems are also found.Conclusions. By increasing the number of known binary orbits by more than one order of magnitude, Gaia DR3 will provide a rich reservoir of dynamical masses and an important contribution to the analysis of stellar multiplicity.
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页数:58
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