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Related papers: Binary and Grouped Open Clusters: A New Catalogue

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Binarity among stellar clusters in galaxy is such a reality which has been realized for a long time, but still hides several questions and problems to be solved. Some of binary star clusters are formed by close encounter, but the others are…

Astrophysics of Galaxies · Physics 2015-06-16 Rhorom Priyatikanto , M. Ikbal Arifyanto , Hesti R. T. Wulandari

Observations indicate that present-day star formation in the Milky Way disk takes place in stellar ensembles or clusters rather than in isolation. Bound, long lived stellar groups are known as open clusters. They gradually lose stars and in…

In dense stellar systems the frequent dynamical interactions between stars play a crucial role in the formation and evolution of compact binaries. We study these processes using a novel approach combining a state-of-the-art binary…

Astrophysics · Physics 2007-05-23 N. Ivanova , F. A. Rasio

Thanks to the recent wide-area photometric surveys, the number of star cluster candidates have risen exponentially in the last few years. Most detections, however, are based only on the presence of an overdensity of stars in a given region,…

Globular clusters are compact, gravitationally bound systems of up to a million stars. The GCs in the Milky Way contain some of the oldest stars known, and provide important clues to the early formation and continuing evolution of our…

Astrophysics of Galaxies · Physics 2020-07-22 Michael A. Beasley

Aims. We estimate the dynamical evolution of the Globular Clusters interaction with the Galactic centre that dynamically changed in the past. Methods. We simulated the orbits of 147 globular clusters over 10 Gyr lookback time using the…

Astrophysics of Galaxies · Physics 2023-06-07 Maryna Ishchenko , Margaryta Sobolenko , Dana Kuvatova , Taras Panamarev , Peter Berczik

We present results constraining the multiplicity of the very low mass stars and sub-stellar objects in the Orion Nebula Cluster (ONC). Our sample covers primary masses 0.012-0.1M$_{\odot}$ using archival Hubble Space Telescope data obtained…

Solar and Stellar Astrophysics · Physics 2022-02-09 Matthew De Furio , Michael R. Meyer , Megan Reiter , John Monnier , Adam Kraus , Trent Dupuy

Close, compact, hierarchical, multiple stellar systems, i.e., multiples having an outer orbital period from months to a few years, comprise a small, but continuously growing group of the triple and multiple star zoo. Many of them consist of…

Solar and Stellar Astrophysics · Physics 2022-01-05 Tamás Borkovits

In this work, we analysed young stellar clusters with spatial and kinematic coherence in the Orion star-forming complex. For this study, we selected a sample of pre-main sequence candidates using parallaxes, proper motions and positions on…

Transiting planets in multiple-star systems, especially high-order multiples, make up a small fraction of the known planet population but provide unique opportunities to study the environments in which planets would have formed.…

We present a suite of direct N-body simulations of low mass ($<10^4~M_{\odot}$) globular cluster streams initialized with observationally-motivated binary demographics in order to understand the effect of in-cluster dynamical processing on…

Astrophysics of Galaxies · Physics 2026-03-10 Anya Phillips , Charlie Conroy , Jacob Nibauer , Long Wang , Vedant Chandra , Ana Bonaca , Jay Strader , Morgan MacLeod

Reconstructing the formation history of the Milky Way is hindered by stellar migration, which erases kinematic birth signatures. In contrast, stellar chemical abundances remain stable and can be used to trace stars back to their birth…

Astrophysics of Galaxies · Physics 2025-10-29 Lorenzo Spina , Milan Quandt Rodriguez , Laura Magrini , Leda Berni , Sara Lucatello , Marco Canducci

Multiple stellar systems are ubiquitous in the Milky Way, but are often unresolved and seen as single objects in spectroscopic, photometric, and astrometric surveys. Yet, modeling them is essential for developing a full understanding of…

Solar and Stellar Astrophysics · Physics 2018-05-02 Axel Widmark , Boris Leistedt , David W. Hogg

We used deep wide field photometric observations to derive the fraction of binary systems in a sample of five high-latitude Galactic open clusters. By analysing the color distribution of Main Sequence stars we derived the minimum fraction…

Solar and Stellar Astrophysics · Physics 2015-05-14 A. Sollima , J. A. Carballo-Bello , G. Beccari , F. R. Ferraro , F. Fusi Pecci , B. Lanzoni

We present the results of time-resolved spectroscopy of 13 O-type stars in the Cas OB6 stellar association. We conducted a survey for radial velocity variability in search of binary systems, which are expected to be plentiful in young OB…

The high-precision {\it Gaia} data release 3 (DR3) enables the discovery of numerous open clusters in the Milky Way, providing an excellent opportunity to search for blue straggler stars in open clusters and investigate their formation and…

Solar and Stellar Astrophysics · Physics 2025-11-11 Songmei Qin , Jing Zhong , Friedrich Anders , Lola Balaguer-Núñez , Chunyan Li , Yueyue Jiang , Guimei Liu , Tong Tang , Li Chen

Dense stellar clusters are natural sites for the origin and evolution of exotic objects such as relativistic binaries (potential gravitational wave sources), blue stragglers, etc. We investigate the secular dynamics of a binary system…

Solar and Stellar Astrophysics · Physics 2019-08-19 Chris Hamilton , Roman R. Rafikov

Binary stars are predicted to have an important role in the evolution of globular clusters, so we obtained binary fractions for 35 globular clusters that were imaged in the F606W and F814W with the ACS on the Hubble Space Telescope. When…

Astrophysics of Galaxies · Physics 2015-05-04 Jun Ji , Joel N. Bregman

Binary stars play a major role in determining the dynamic evolution of star clusters. We used images collected with the Hubble Space Telescope to study fourteen Magellanic Clouds star clusters that span an age interval between $\sim 0.6$…

Context. Stars are born together from giant molecular clouds and, if we assume that the priors were chemically homogeneous and well-mixed, we expect them to share the same chemical composition. Most of the stellar aggregates are disrupted…