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The second Gaia data release (Gaia DR2) provided us with the precise five-parameter astrometry for 1.3 billion of sources. As stars passing close to the Solar System are thought to be responsible for influencing the dynamical history of…

地球与行星天体物理 · 物理学 2022-01-31 Rita Wysoczańska , Piotr A. Dybczyński , Magdalena Polińska

Passing stars may play an important role in the evolution of our solar system. We search for close stellar encounters to the Sun among all 7.2 million stars in Gaia-DR2 that have six-dimensional phase space data. We characterize encounters…

太阳与恒星天体物理 · 物理学 2018-08-15 C. A. L. Bailer-Jones , J. Rybizki , R. Andrae , M. Fouesneau

In the latest Gaia third data release one can find extremely small proper motion components for the star HD 7977. This, together with the radial velocity measurement lead to the conclusion that this star passed very close to the Sun in the…

We have studied stellar candidates for close (within 1 pc) encounters with the Solar system. For all of the stars under consideration the kinematic characteristics have been taken from the Gaia EDR3 catalogue. The parameters of the…

星系天体物理 · 物理学 2021-04-22 Vadim V. Bobylev , Anisa T. Bajkova

Close encounters of stars to the Sun could affect life on Earth through gravitational perturbations of comets in the Oort cloud or exposure to ionizing radiation. By integrating orbits through the Galactic potential, I identify which of 33…

太阳与恒星天体物理 · 物理学 2022-08-24 C. A. L. Bailer-Jones

Aims. We introduce a novel way to identify new compact hierarchical triple stars by exploiting the huge potential of Gaia DR3 and also its future data releases. We aim to increase the current number of compact hierarchical triples…

A search for close encounters of stars with the Solar System was performed using data from the Gaia\,DR3 catalog. We considered 31 stars with the approach parameter $d_{\rm min}<1$~pc. Among them, 15 stars are appearing as candidates for…

星系天体物理 · 物理学 2023-05-23 Vadim Bobylev , Anisa Bajkova

I report on close encounters of stars to the Sun found in the first Gaia data release (GDR1). Combining Gaia astrometry with radial velocities of around 320 000 stars drawn from various catalogues, I integrate orbits in a Galactic potential…

太阳与恒星天体物理 · 物理学 2018-01-10 C. A. L. Bailer-Jones

We have searched for the stars that either encountered in the past or will encounter in the future with the Solar system closer than 2 pc. For this purpose, we took more than 216 000 stars with the measured proper motions and trigonometric…

星系天体物理 · 物理学 2017-06-28 V. V. Bobylev , A. T. Bajkova

The multiplicity fraction of stars, down to the substellar regime, is a parameter of fundamental importance for stellar formation, evolution, and planetology. The census of multiple stars in the solar neighborhood is however incomplete. Our…

太阳与恒星天体物理 · 物理学 2021-12-22 Pierre Kervella , Frédéric Arenou , Frédéric Thévenin

We produce a clean and well-characterised catalogue of objects within 100\,pc of the Sun from the \G\ Early Data Release 3. We characterise the catalogue through comparisons to the full data release, external catalogues, and simulations. We…

太阳与恒星天体物理 · 物理学 2021-04-28 Gaia Collaboration , R. L. Smart , L. M. Sarro , J. Rybizki , C. Reylé , A. C. Robin , N. C. Hambly , U. Abbas , M. A. Barstow , J. H. J. de Bruijne , B. Bucciarelli , J. M. Carrasco , W. J. Cooper , S. T. Hodgkin , E. Masana , D. Michalik , J. Sahlmann , A. Sozzetti , A. G. A. Brown , A. Vallenari , T. Prusti , C. Babusiaux , M. Biermann , O. L. Creevey , D. W. Evans , L. Eyer , A. Hutton , F. Jansen , C. Jordi , S. A. Klioner , U. Lammers , L. Lindegren , X. Luri , F. Mignard , C. Panem , D. Pourbaix , S. Randich , P. Sartoretti , C. Soubiran , N. A. Walton , F. Arenou , C. A. L. Bailer-Jones , U. Bastian , M. Cropper , R. Drimmel , D. Katz , M. G. Lattanzi , F. van Leeuwen , J. Bakker , J. Castañeda , F. De Angeli , C. Ducourant , C. Fabricius , M. Fouesneau , Y. Frémat , R. Guerra , A. Guerrier , J. Guiraud , A. Jean-Antoine Piccolo , R. Messineo , N. Mowlavi , C. Nicolas , K. Nienartowicz , F. Pailler , P. Panuzzo , F. Riclet , W. Roux , G. M. Seabroke , R. Sordo , P. Tanga , F. Thévenin , G. Gracia-Abril , J. Portell , D. Teyssier , M. Altmann , R. Andrae , I. Bellas-Velidis , K. Benson , J. Berthier , R. Blomme , E. Brugaletta , P. W. Burgess , G. Busso , B. Carry , A. Cellino , N. Cheek , G. Clementini , Y. Damerdji , M. Davidson , L. Delchambre , A. Dell'Oro , J. Fernández-Hernández , L. Galluccio , P. García-Lario , M. Garcia-Reinaldos , J. González-Núñez , E. Gosset , R. Haigron , J. -L. Halbwachs , D. L. Harrison , D. Hatzidimitriou , U. Heiter , J. Hernández , D. Hestroffer , B. Holl , K. Janßen , G. Jevardat de Fombelle , S. Jordan , A. Krone-Martins , A. C. Lanzafame , W. Löffler , A. Lorca , M. Manteiga , O. Marchal , P. M. Marrese , A. Moitinho , A. Mora , K. Muinonen , P. Osborne , E. Pancino , T. Pauwels , A. Recio-Blanco , P. J. Richards , M. Riello , L. Rimoldini , T. Roegiers , C. Siopis , M. Smith , A. Ulla , E. Utrilla , M. van Leeuwen , W. van Reeven , A. Abreu Aramburu , S. Accart , C. Aerts , J. J. Aguado , M. Ajaj , G. Altavilla , M. A. Álvarez , J. Álvarez Cid-Fuentes , J. Alves , R. I. Anderson , E. Anglada Varela , T. Antoja , M. Audard , D. Baines , S. G. Baker , L. Balaguer-Núñez , E. Balbinot , Z. Balog , C. Barache , D. Barbato , M. Barros , S. Bartolomé , J. -L. Bassilana , N. Bauchet , A. Baudesson-Stella , U. Becciani , M. Bellazzini , M. Bernet , S. Bertone , L. Bianchi , S. Blanco-Cuaresma , T. Boch , A. Bombrun , D. Bossini , S. Bouquillon , A. Bragaglia , L. Bramante , E. Breedt , A. Bressan , N. Brouillet , A. Burlacu , D. Busonero , A. G. Butkevich , R. Buzzi , E. Caffau , R. Cancelliere , H. Cánovas , T. Cantat-Gaudin , R. Carballo , T. Carlucci , M. I Carnerero , L. Casamiquela , M. Castellani , A. Castro-Ginard , P. Castro Sampol , L. Chaoul , P. Charlot , L. Chemin , A. Chiavassa , M. -R. L. Cioni , G. Comoretto , T. Cornez , S. Cowell , F. Crifo , M. Crosta , C. Crowley , C. Dafonte , A. Dapergolas , M. David , P. David , P. de Laverny , F. De Luise , R. De March , J. De Ridder , R. de Souza , P. de Teodoro , A. de Torres , E. F. del Peloso , E. del Pozo , A. Delgado , H. E. Delgado , J. -B. Delisle , P. Di Matteo , S. Diakite , C. Diener , E. Distefano , C. Dolding , D. Eappachen , B. Edvardsson , H. Enke , P. Esquej , C. Fabre , M. Fabrizio , S. Faigler , G. Fedorets , P. Fernique , A. Fienga , F. Figueras , C. Fouron , F. Fragkoudi , E. Fraile , F. Franke , M. Gai , D. Garabato , A. Garcia-Gutierrez , M. García-Torres , A. Garofalo , P. Gavras , E. Gerlach , R. Geyer , P. Giacobbe , G. Gilmore , S. Girona , G. Giuffrida , R. Gomel , A. Gomez , I. Gonzalez-Santamaria , J. J. González-Vidal , M. Granvik , R. Gutiérrez-Sánchez , L. P. Guy , M. Hauser , M. Haywood , A. Helmi , S. L. Hidalgo , T. Hilger , N. Hładczuk , D. Hobbs , G. Holland , H. E. Huckle , G. Jasniewicz , P. G. Jonker , J. Juaristi Campillo , F. Julbe , L. Karbevska , P. Kervella , S. Khanna , A. Kochoska , M. Kontizas , G. Kordopatis , A. J. Korn , Z. Kostrzewa-Rutkowska , K. Kruszyńska , S. Lambert , A. F. Lanza , Y. Lasne , J. -F. Le Campion , Y. Le Fustec , Y. Lebreton , T. Lebzelter , S. Leccia , N. Leclerc , I. Lecoeur-Taibi , S. Liao , E. Licata , H. E. P. Lindstrøm , T. A. Lister , E. Livanou , A. Lobel , P. Madrero Pardo , S. Managau , R. G. Mann , J. M. Marchant , M. Marconi , M. M. S. Marcos Santos , S. Marinoni , F. Marocco , D. J. Marshall , L. Martin Polo , J. M. Martín-Fleitas , A. Masip , D. Massari , A. Mastrobuono-Battisti , T. Mazeh , P. J. McMillan , S. Messina , N. R. Millar , A. Mints , D. Molina , R. Molinaro , L. Molnár , P. Montegriffo , R. Mor , R. Morbidelli , T. Morel , D. Morris , A. F. Mulone , D. Munoz , T. Muraveva , C. P. Murphy , I. Musella , L. Noval , C. Ordénovic , G. Orrù , J. Osinde , C. Pagani , I. Pagano , L. Palaversa , P. A. Palicio , A. Panahi , M. Pawlak , X. Peñalosa Esteller , A. Penttilä , A. M. Piersimoni , F. -X. Pineau , E. Plachy , G. Plum , E. Poggio , E. Poretti , E. Poujoulet , A. Prša , L. Pulone , E. Racero , S. Ragaini , M. Rainer , C. M. Raiteri , N. Rambaux , P. Ramos , M. Ramos-Lerate , P. Re Fiorentin , S. Regibo , V. Ripepi , A. Riva , G. Rixon , N. Robichon , C. Robin , M. Roelens , L. Rohrbasser , M. Romero-Gómez , N. Rowell , F. Royer , K. A. Rybicki , G. Sadowski , A. Sagristà Sellés , J. Salgado , E. Salguero , N. Samaras , V. Sanchez Gimenez , N. Sanna , R. Santoveña , M. Sarasso , M. Schultheis , E. Sciacca , M. Segol , J. C. Segovia , D. Ségransan , D. Semeux , S. Shahaf , H. I. Siddiqui , A. Siebert , L. Siltala , E. Slezak , E. Solano , F. Solitro , D. Souami , J. Souchay , A. Spagna , F. Spoto , I. A. Steele , H. Steidelmüller , C. A. Stephenson , M. Süveges , L. Szabados , E. Szegedi-Elek , F. Taris , G. Tauran , M. B. Taylor , R. Teixeira , W. Thuillot , N. Tonello , F. Torra , J. Torra , C. Turon , N. Unger , M. Vaillant , E. van Dillen , O. Vanel , A. Vecchiato , Y. Viala , D. Vicente , S. Voutsinas , M. Weiler , T. Wevers , L. Wyrzykowski , A. Yoldas , P. Yvard , H. Zhao , J. Zorec , S. Zucker , C. Zurbach , T. Zwitter

In light of substantial new discoveries of hot subdwarfs by ongoing spectroscopic surveys and the availability of the Gaia mission Early Data Release 3 (EDR3), we compiled new releases of two catalogues of hot subluminous stars: The data…

太阳与恒星天体物理 · 物理学 2022-06-15 Richard Culpan , Stephan Geier , Ingrid Pelisoli , Nicole Reindl , Nicola Gentile Fusillo , Alina Vorontseva

We present a catalog of unbound stellar pairs, within 100 pc of the Sun, that are undergoing close, hyperbolic, encounters. The data are drawn from the GAIA EDR3 catalogue, and the limiting factors are errors in the radial distance and…

太阳与恒星天体物理 · 物理学 2022-01-12 Bradley M. S. Hansen

We consider 36 candidates for close (within 1 pc) encounters with the Solar system. These stars have been selected in accordance with the results of an analysis of their motion obtained by various authors. For most stars from this list the…

星系天体物理 · 物理学 2020-07-01 V. V. Bobylev , A. T. Bajkova

The early third data release (EDR3) of the European Space Agency satellite Gaia provides coordinates, parallaxes, and proper motions for ~1.47 billion sources in our Milky Way, based on 34 months of observations. The combination of Gaia DR2…

星系天体物理 · 物理学 2021-03-17 Tommaso Marchetti

The aim of this paper is to demonstrate the accuracy of our knowledge of close stellar passage distances in the pre-GAIA era.We used the most precise astrometric and kinematic data available at the moment and prepared a list of 40 stars…

地球与行星天体物理 · 物理学 2015-06-23 Piotr A. Dybczyński , Filip Berski

Context. Planetary nebulae (PNe) are a brief but important phase of stellar evolution. The study of Galactic PNe has historically been hampered by uncertain distances, but the parallaxes of PN central stars (CSPNe) measured by Gaia are…

太阳与恒星天体物理 · 物理学 2021-12-11 N. Chornay , N. A. Walton

Since 1950 when Oort published his paper on the structure of the cloud of comets it is believed that stars passing near this hypothetical cometary reservoir play an important role in the dynamical evolution of long period comets and…

地球与行星天体物理 · 物理学 2020-01-08 Rita Wysoczańska , Piotr A. Dybczyński , Małgorzata Królikowska

We present a catalog of 3354 candidate young stars within 500 pc that appear to have been ejected from their parent associations with relative speeds of >5 km/s. These candidates have been homogeneously selected through performing a 2d…

太阳与恒星天体物理 · 物理学 2022-10-12 Marina Kounkel , Aidan McBride , Keivan G. Stassun , Nathan Leigh

The census of stellar and substellar companions of nearby stars is largely incomplete. It is, however, fundamentally important in the understanding of the stellar and planetary formation and evolution mechanisms. We aim to characterize the…

太阳与恒星天体物理 · 物理学 2019-03-06 Pierre Kervella , Frédéric Arenou , François Mignard , Frédéric Thévenin
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