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Related papers: Stellar clusters in the Gaia era

200 papers

The Gaia-ESO Survey (GES) is a large public spectroscopic survey that aims at observing with FLAMES@VLT the main stellar components of our Galaxy. The study of the population of open clusters is one of the main objectives of GES. We present…

Astrophysics of Galaxies · Physics 2015-06-01 Laura Magrini , Sofia Randich

We use the framework developed as part of the MESA Isochrones and Stellar Tracks (MIST) project to assess the utility of several types of observables in jointly measuring the age and 1D stellar model parameters in star clusters. We begin…

Solar and Stellar Astrophysics · Physics 2018-08-15 Jieun Choi , Charlie Conroy , Yuan-Sen Ting , Phillip A. Cargile , Aaron Dotter , Benjamin D. Johnson

Globular clusters are stellar dynamical systems which evolve on stellar evolutionary and both internal and external dynamical timescales. Quantitative comparison of cluster properties with realistic evolutionary dynamical models is becoming…

Astrophysics · Physics 2007-05-23 Gerard Gilmore

Open and globular star clusters have served as benchmarks for the study of stellar evolution due to their supposed nature as simple stellar populations of the same age and metallicity. After a brief review of some of the pioneering work…

Astrophysics of Galaxies · Physics 2015-05-14 Jason S. Kalirai , Harvey B. Richer

Open clusters are convenient probes of the structure and history of the Galactic disk. They are also fundamental to stellar evolution studies. The second Gaia data release contains precise astrometry at the sub-milliarcsecond level and…

Stellar populations, building blocks of galaxies, are direct tracers of the star formation history, the chemical enrichment and the assembly of galaxies in the Universe. They therfore allow us to understand how galaxies formed and evolved.…

Astrophysics · Physics 2007-07-30 A. Vazdekis , R. F. Peletier

The Gaia benchmark stars are stars with very precise stellar parameters that cover a wide range in the HR diagram at various metallicities. They are meant to be good representative of typical FGK stars in the Milky Way. Currently, they are…

Solar and Stellar Astrophysics · Physics 2016-10-19 Paula Jofre

In this contribution I provide a brief summary of the contents of Gaia DR1. This is followed by a discussion of studies in the literature that attempt to characterize the quality of the Tycho-Gaia Astrometric Solution parallaxes in Gaia…

Astrophysics of Galaxies · Physics 2018-06-13 Anthony G. A. Brown

Ages are key to truly understand a large plethora of astrophysical phenomena. On the other hand, stellar clusters are open windows to understand stellar evolution, specifically, the change with time and mass of different stellar properties.…

Solar and Stellar Astrophysics · Physics 2016-11-23 David Barrado

Globular clusters play a role in many areas of astrophysics, ranging from stellar physics to cosmology. New ground-based optical surveys complemented by observations from space-based telescopes with unprecedented near-infrared capabilities…

The Gaia mission is reviewed together with the expected contents of the final catalogue. It is then argued that the ultimate goal of Galactic structure studies with Gaia astrometry should be to build a dynamical model of our galaxy which is…

Astrophysics · Physics 2009-11-13 Anthony G. A. Brown

Combined studies of variable stars and stellar clusters open great horizons, and they allow us to improve our understanding of stellar cluster formation and stellar evolution. In that prospect, the Gaia mission will provide astrometric,…

In the last 15 years different ground-based spectroscopic surveys have been started (and completed) with the general aim of delivering stellar parameters and elemental abundances for large samples of Galactic stars, complementing Gaia…

Astrophysics of Galaxies · Physics 2022-10-26 S. Randich , G. Gilmore , L. Magrini , G. G. Sacco , R. J. Jackson , R. D. Jeffries , C. C. Worley , A. Hourihane , A. Gonneau , C. Viscasillas Vàzquez , E. Franciosini , J. R. Lewis , E. J. Alfaro , C. Allende Prieto , T. Bensby R. Blomme , A. Bragaglia , E. Flaccomio , P. François , M. J. Irwin , S. E. Koposov , A. J. Korn , A. C. Lanzafame , E. Pancino , A. Recio-Blanco , R. Smiljanic , S. Van Eck , T. Zwitter , M. Asplund , P. Bonifacio , S. Feltzing , J. Binney , J. Drew , A. M. N. Ferguson , G. Micela , I. Negueruela , T. Prusti , H. -W. Rix , A. Vallenari , A. Bayo , M. Bergemann , K. Biazzo , G. Carraro , A. R. Casey , F. Damiani , A. Frasca , U. Heiter , V. Hill , P. Jofré , P. de Laverny , K. Lind , G. Marconi , C. Martayan , T. Masseron , L. Monaco , L. Morbidelli , L. Prisinzano , L. Sbordone , S. G. Sousa , S. Zaggia , V. Adibekyan , R. Bonito , E. Caffau , S. Daflon , D. K. Feuillet , M. Gebran , J. I. González Hernández , G. Guiglion , A. Herrero , A. Lobel , J. Maíz Apellániz , T. Merle , S. Mikolaitis , D. Montes , T. Morel , C. Soubiran , L. Spina , H. M. Tabernero , G. Tautvaišienė , G. Traven , M. Valentini , M. Van der Swaelmen , S. Villanova , N. J. Wright , U. Abbas , V. Aguirre Børsen-Koch , J. Alves , L. Balaguer-Núnez , P. S. Barklem , D. Barrado , S. R. Berlanas , A. S. Binks , A. Bressan , R. Capuzzo--Dolcetta , L. Casagrande , L. Casamiquela , R. S. Collins , V. D'Orazi , M. L. L. Dantas , V. P. Debattista , E. Delgado-Mena , P. Di Marcantonio , A. Drazdauskas , N. W. Evans , B. Famaey , M. Franchini , Y. Frémat , E. D. Friel , X. Fu , D. Geisler , O. Gerhard , E. A. González Solares , E. K. Grebel , M. L. Gutiérrez Albarrán , D. Hatzidimitriou , E. V. Held , F. Jiménez-Esteban , H. Jönsson , C. Jordi , T. Khachaturyants , G. Kordopatis , J. Kos , N. Lagarde , L. Mahy , M. Mapelli , E. Marfil , S. L. Martell , S. Messina , A. Miglio , I. Minchev , A. Moitinho , J. Montalban , M. J. P. F. G. Monteiro , C. Morossi , N. Mowlavi , A. Mucciarelli , D. N. A. Murphy , N. Nardetto , S. Ortolani , F. Paletou , J. Palouus , E. Paunzen , J. C. Pickering , A. Quirrenbach , P. Re Fiorentin , J. I. Read , D. Romano , N. Ryde , N. Sanna , W. Santos , G. M. Seabroke , A. Spagna , M. Steinmetz , E. Stonkuté , E. Sutorius , F. Thévenin , M. Tosi , M. Tsantaki , J. S. Vink , N. Wright , R. F. G. Wyse , M. Zoccali , J. Zorec , D. B. Zucker , N. A. Walton

The study of open star clusters makes us understand a lot about the composition and construction of the Milky Way Galaxy. Thanks to the Gaia DR2 database that helps us to get the genetic members of star clusters using their proper motions…

Astrophysics of Galaxies · Physics 2021-09-23 W. A. Badawy , A. L. Tadross , Y. M. Hendy , I. A. Hassan , M. N. Ismail

Gaia is a satellite mission of the European Space Agency which is creating a catalogue of extremely accurate positions, distances and space motions of two billion stars in our Galaxy, along with more than one hundred thousand solar system…

Instrumentation and Methods for Astrophysics · Physics 2025-09-16 Michael Perryman

It is widely accepted that stars do not form in isolation but result from the fragmentation of molecular clouds, which in turn leads to star cluster formation. Over time, clusters dissolve or are destroyed by interactions with molecular…

The Gaia data will help to improve the construction of a luminosity function for the disk and the halo and will provide a more accurate determination of the age of our solar neighborhood. Moreover, reliable stellar dynamical investigations…

Astrophysics · Physics 2007-05-23 Stefan Jordan

Stellar multiplicity is among the oldest and richest problems in astrophysics. Binary stars are a cornerstone of stellar mass and radius measurements that underpin modern stellar evolutionary models. Binaries are the progenitors of many of…

Solar and Stellar Astrophysics · Physics 2024-05-15 Kareem El-Badry

Globular clusters are highly efficient radio pulsar factories. These pulsars can be used as precision probes of the clusters' structure, gas content, magnetic field, and formation history; some of them are also highly interesting in their…

High Energy Astrophysical Phenomena · Physics 2015-01-05 J. W. T. Hessels , A. Possenti , M. Bailes , C. G. Bassa , P. C. C. Freire , D. R. Lorimer , R. Lynch , S. M. Ransom , I. H. Stairs

We present the results of a systematic Milky Way satellite search performed across an array of publicly available wide-area photometric surveys. Our aim is to complement previous searches by widening the parameter space covered.…

Astrophysics of Galaxies · Physics 2019-01-28 G. Torrealba , V. Belokurov , S. E. Koposov