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2023A&A...674A..34G - Astronomy and Astrophysics, volume 674A34 (2023/6-1)
Gaia Data Release 3 Stellar multiplicity, a teaser for the hidden treasure.
GAIA COLLABORATION, ARENOU F., BABUSIAUX C., BARSTOW M.A., FAIGLER S., JORISSEN A., KERVELLA P., MAZEH T., MOWLAVI N., PANUZZO P., SAHLMANN J., SHAHAF S., SOZZETTI A., BAUCHET N., DAMERDJI Y., GAVRAS P., GIACOBBE P., GOSSET E., HALBWACHS J.-L., HOLL B., LATTANZI M.G., LECLERC N., MOREL T., POURBAIX D., RE FIORENTIN P., SADOWSKI G., SEGRANSAN D., SIOPIS C., TEYSSIER D., ZWITTER T., PLANQUART L., BROWN A.G.A., VALLENARI A., PRUSTI T., DE BRUIJNE J.H.J., BIERMANN M., CREEVEY O.L., DUCOURANT C., EVANS D.W., EYER L., GUERRA R., HUTTON A., JORDI C., KLIONER S.A., LAMMERS U.L., LINDEGREN L., LURI X., MIGNARD F., PANEM C., RANDICH S., SARTORETTI P., SOUBIRAN C., TANGA P., WALTON N.A., BAILER-JONES C.A.L., BASTIAN U., DRIMMEL R., JANSEN F., KATZ D., VAN LEEUWEN F., BAKKER J., CACCIARI C., CASTANEDA J., DE ANGELI F., FABRICIUS C., FOUESNEAU M., FREMAT Y., GALLUCCIO L., GUERRIER A., HEITER U., MASANA E., MESSINEO R., NICOLAS C., NIENARTOWICZ K., PAILLER F., RICLET F., ROUX W., SEABROKE G.M., SORDO R., THEVENIN F., GRACIA-ABRIL G., PORTELL J., ALTMANN M., ANDRAE R., AUDARD M., BELLAS-VELIDIS I., BENSON K., BERTHIER J., BLOMME R., BURGESS P.W., BUSONERO D., BUSSO G., CANOVAS H., CARRY B., CELLINO A., CHEEK N., CLEMENTINI G., DAVIDSON M., DE TEODORO P., NUNEZ CAMPOS M., DELCHAMBRE L., DELL'ORO A., ESQUEJ P., FERNANDEZ-HERNANDEZ J., FRAILE E., GARABATO D., GARCIA-LARIO P., HAIGRON R., HAMBLY N.C., HARRISON D.L., HERNANDEZ J., HESTROFFER D., HODGKIN S.T., JANSSEN K., JEVARDAT DE FOMBELLE G., JORDAN S., KRONE-MARTINS A., LANZAFAME A.C., LOFFLER W., MARCHAL O., MARRESE P.M., MOITINHO A., MUINONEN K., OSBORNE P., PANCINO E., PAUWELS T., RECIO-BLANCO A., REYLE C., RIELLO M., RIMOLDINI L., ROEGIERS T., RYBIZKI J., SARRO L.M., SMITH M., UTRILLA E., VAN LEEUWEN M., ABBAS U., ABRAHAM P., ABREU ARAMBURU A., AERTS C., AGUADO J.J., AJAJ M., ALDEA-MONTERO F., ALTAVILLA G., ALVAREZ M.A., ALVES J., ANDERS F., ANDERSON R.I., ANGLADA VARELA E., ANTOJA T., BAINES D., BAKER S.G., BALAGUER-NUNEZ L., BALBINOT E., BALOG Z., BARACHE C., BARBATO D., BARROS M., BARTOLOME S., BASSILANA J.-L., BECCIANI U., BELLAZZINI M., BERIHUETE A., BERNET M., BERTONE S., BIANCHI L., BINNENFELD A., BLANCO-CUARESMA S., BLAZERE A., BOCH T., BOMBRUN A., BOSSINI D., BOUQUILLON S., BRAGAGLIA A., BRAMANTE L., BREEDT E., BRESSAN A., BROUILLET N., BRUGALETTA E., BUCCIARELLI B., BURLACU A., BUTKEVICH A.G., BUZZI R., CAFFAU E., CANCELLIERE R., CANTAT-GAUDIN T., CARBALLO R., CARLUCCI T., CARNERERO M.I., CARRASCO J.M., CASAMIQUELA L., CASTELLANI M., CASTRO-GINARD A., CHAOUL L., CHARLOT P., CHEMIN L., CHIARAMIDA V., CHIAVASSA A., CHORNAY N., COMORETTO G., CONTURSI G., COOPER W.J., CORNEZ T., COWELL S., CRIFO F., CROPPER M., CROSTA M., CROWLEY C., DAFONTE C., DAPERGOLAS A., DAVID P., DE LAVERNY P., DE LUISE F., DE MARCH R., DE RIDDER J., DE SOUZA R., DE TORRES A., DEL PELOSO E.F., DEL POZO E., DELBO M., DELGADO A., DELISLE J.-B., DEMOUCHY C., DHARMAWARDENA T.E., DIAKITE S., DIENER C., DISTEFANO E., DOLDING C., ENKE H., FABRE C., FABRIZIO M., FEDORETS G., FERNIQUE P., FIGUERAS F., FOURNIER Y., FOURON C., FRAGKOUDI F., GAI M., GARCIA-GUTIERREZ A., GARCIA-REINALDOS M., GARCIA-TORRES M., GAROFALO A., GAVEL A., GERLACH E., GEYER R., GILMORE G., GIRONA S., GIUFFRIDA G., GOMEL R., GOMEZ A., GONZALEZ-NUNEZ J., GONZALEZ-SANTAMARIA I., GONZALEZ-VIDAL J.J., GRANVIK M., GUILLOUT P., GUIRAUD J., GUTIERREZ-SANCHEZ R., GUY L.P., HATZIDIMITRIOU D., HAUSER M., HAYWOOD M., HELMER A., HELMI A., SARMIENTO M.H., HIDALGO S.L., HILGER T., HLADCZUK N., HOBBS D., HOLLAND G., HUCKLE H.E., JARDINE K., JASNIEWICZ G., JEAN-ANTOINE PICCOLO A., JIMENEZ-ARRANZ O., JUARISTI CAMPILLO J., JULBE F., KARBEVSKA L., KHANNA S., KORDOPATIS G., KORN A.J., KOSPAL A., KOSTRZEWA-RUTKOWSKA Z., KRUSZYNSKA K., KUN M., LAIZEAU P., LAMBERT S., LANZA A.F., LASNE Y., LE CAMPION J.-F., LEBRETON Y., LEBZELTER T., LECCIA S., LECOEUR-TAIBI I., LIAO S., LICATA E.L., LINDSTROM H.E.P., LISTER T.A., LIVANOU E., LOBEL A., LORCA A., LOUP C., MADRERO PARDO P., MAGDALENO ROMEO A., MANAGAU S., MANN R.G., MANTEIGA M., MARCHANT J.M., MARCONI M., MARCOS J., MARCOS SANTOS M.M.S., MARIN PINA D., MARINONI S., MAROCCO F., MARSHALL D.J., MARTIN POLO L., MARTIN-FLEITAS J.M., MARTON G., MARY N., MASIP A., MASSARI D., MASTROBUONO-BATTISTI A., McMILLAN P.J., MESSINA S., MICHALIK D., MILLAR N.R., MINTS A., MOLINA D., MOLINARO R., MOLNAR L., MONARI G., MONGUIO M., MONTEGRIFFO P., MONTERO A., MOR R., MORA A., MORBIDELLI R., MORRIS D., MURAVEVA T., MURPHY C.P., MUSELLA I., NAGY Z., NOVAL L., OCANA F., OGDEN A., ORDENOVIC C., OSINDE J.O., PAGANI C., PAGANO I., PALAVERSA L., PALICIO P.A., PALLAS-QUINTELA L., PANAHI A., PAYNE-WARDENAAR S., PENALOSA ESTELLER X., PENTTILA A., PICHON B., PIERSIMONI A.M., PINEAU F.-X., PLACHY E., PLUM G., POGGIO E., PRSA A., PULONE L., RACERO E., RAGAINI S., RAINER M., RAITERI C.M., RAMOS P., RAMOS-LERATE M., REGIBO S., RICHARDS P.J., RIOS DIAZ C., RIPEPI V., RIVA A., RIX H.-W., RIXON G., ROBICHON N., ROBIN A.C., ROBIN C., ROELENS M., ROGUES H.R.O., ROHRBASSER L., ROMERO-GOMEZ M., ROWELL N., ROYER F., RUZ MIERES D., RYBICKI K.A., SAEZ NUNEZ A., SAGRISTA SELLES A., SALGUERO E., SAMARAS N., SANCHEZ GIMENEZ V., SANNA N., SANTOVENA R., SARASSO M., SCHULTHEIS M., SCIACCA E., SEGOL M., SEGOVIA J.C., SEMEUX D., SIDDIQUI H.I., SIEBERT A., SILTALA L., SILVELO A., SLEZAK E., SLEZAK I., SMART R.L., SNAITH O.N., SOLANO E., SOLITRO F., SOUAMI D., SOUCHAY J., SPAGNA A., SPINA L., SPOTO F., STEELE I.A., STEIDELMULLER H., STEPHENSON C.A., SUVEGES M., SURDEJ J., SZABADOS L., SZEGEDI-ELEK E., TARIS F., TAYLOR M.B., TEIXEIRA R., TOLOMEI L., TONELLO N., TORRA F., TORRA J., TORRALBA ELIPE G., TRABUCCHI M., TSOUNIS A.T., TURON C., ULLA A., UNGER N., VAILLANT M.V., VAN DILLEN E., VAN REEVEN W., VANEL O., VECCHIATO A., VIALA Y., VICENTE D., VOUTSINAS S., WEILER M., WEVERS T., WYRZYKOWSKI L., YOLDAS A., YVARD P., ZHAO H., ZOREC J. and ZUCKER S.
Abstract (from CDS):
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.
Abstract Copyright: © The Authors 2023
Journal keyword(s): binaries: general - astrometry - planetary systems - stars: fundamental parameters - catalogs - white dwarfs
VizieR on-line data: See catalogue I/357 (Gaia DR3 Part 3. Non-single stars. 2022yCat.1357....0G)
Status at CDS : All or part of tables of objects could be ingested in SIMBAD; there are some issues with cross-identifications or classifications.
CDS comments: Eclipsing (EB*) and Spectroscopic (SB*) Binaries are ingested in SIMBAD (from VizieR tables : I/357/tboeb , I/357/tboes , I/357/tboasb1c , I/357/tbosb1 , I/357/tbosb1c , I/357/tbosb2 , I/357/tbosb2c). Like for variable star surveys, the orbital period is recorded in the Collection of Measurements Var (see http://simbad.cds.unistra.fr/simbad/sim-display?data=meas#v* ; vartyp coded as E , SB-E , SB1-AB , SB1 , SB1C , SB2 , SB2C , respectively).
Simbad objects: 307215
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