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A method to search for tidal streams and to fit their orbits based on maximum likelihood is presented and applied to the Gaia data. Tests of the method are performed showing how a simulated stream produced by tidal stripping of a star…

星系天体物理 · 物理学 2020-10-28 C. G. Palau , J. Miralda-Escudé

The hierarchical model of galaxy formation predicts that the Milky Way halo is populated by tidal debris of dwarf galaxies and globular clusters. Due to long dynamical times, debris from the lowest mass objects remains coherent as thin and…

星系天体物理 · 物理学 2024-05-31 Ana Bonaca , Adrian M. Price-Whelan

We apply the automatic stellar stream detection algorithm StarStream to Gaia Data Release 3 and identify 87 stellar streams associated with Galactic globular clusters (GCs), including 34 high-quality cases with median completeness and…

星系天体物理 · 物理学 2026-03-02 Yingtian Chen , Oleg Y. Gnedin , Adrian M. Price-Whelan

The Gaia mission promises to deliver precision astrometry at an unprecedented level, heralding a new era for discerning the kinematic and spatial coordinates of stars in our Galaxy. Here, we present a new technique for estimating the age of…

星系天体物理 · 物理学 2018-06-06 Sownak Bose , Idan Ginsburg , Abraham Loeb

The Gaia mission has led to the discovery of over 100 stellar streams in the Milky Way, most of which likely originated from globular clusters (GCs). As the upcoming wide-field surveys can potentially continue to increase the number of…

星系天体物理 · 物理学 2025-12-12 Yingtian Chen , Oleg Y. Gnedin , Adrian M. Price-Whelan , Colin Holm-Hansen

We propose an extension of the GC3 streamer finding method of Johnston et al. 1996 that can be applied to the future Gaia database. The original method looks for streamers along great circles in the sky, our extension adds the kinematical…

In the coming decade the Gaia satellite will precisely measure the positions and velocities of millions of stars in the Galactic halo, including stars in many tidal streams. These streams, the products of hierarchical accretion of satellite…

星系天体物理 · 物理学 2016-02-17 Robyn E. Sanderson

Thanks to the precise astrometric measurements of proper motions by the Gaia mission, a new tidal stellar stream has been discovered in the northern hemisphere. The distribution of star count shows that the stream is approximately $80$…

星系天体物理 · 物理学 2024-04-09 Hao Tian , Chao Liu , Changqing Luo , Xiang-Xiang Xue , Yujiao Yang

We present an atlas and follow-up spectroscopic observations of 87 thin stream-like structures detected with the STREAMFINDER algorithm in Gaia DR3, of which 29 are new discoveries. Here we focus on using these streams to refine mass models…

We address the problem of identifying remnants of satellite galaxies in the halo of our galaxy with Gaia data. The remnants have to be extracted from a very large data set (of order 10^9 stars) in the presence of observational errors and…

天体物理学 · 物理学 2009-11-11 Anthony Brown , Hector Velazquez , Luis Aguilar , ;

We present a panoramic map of the stellar streams of the Milky Way based upon astrometric and photometric measurements from the Gaia DR2 catalogue. In this first contribution, we concentrate on the halo at heliocentric distances beyond 5…

星系天体物理 · 物理学 2018-09-19 Khyati Malhan , Rodrigo A. Ibata , Nicolas F. Martin

We explore the use of tidal streams from Galactic satellites to recover the potential of the Milky Way. Our study is motivated both by the discovery of the first lengthy stellar stream in the halo (\cite{it98}) and by the prospect of…

天体物理学 · 物理学 2009-10-30 Kathryn V. Johnston , HongSheng Zhao , David N. Spergel , Lars Hernquist

We investigate what the proposed ESA astrometric satellite GAIA will reveal by observing the halo of the Milky Way. Specifically, we look for halo streams which are the signatures left by the merging/accretion events experienced by a…

天体物理学 · 物理学 2007-05-23 Amina Helmi , HongSheng Zhao , P. Tim de Zeeuw

I analyse the projected density distribution of member stars over a wide area surrounding 18 Galactic globular clusters using the photometric and astrometric information provided by the second data release of the Gaia mission. A 5D mixture…

星系天体物理 · 物理学 2020-05-27 A. Sollima

Streams of stars from captured dwarf galaxies and dissolved globular clusters are identifiable through the similarity of their orbital parameters, a fact that remains true long after the streams have dispersed spatially. We calculate the…

星系天体物理 · 物理学 2020-01-08 Nicholas W. Borsato , Sarah L. Martell , Jeffrey D. Simpson

Dynamically cold stellar streams from tidally dissolved globular clusters (GCs) serve as excellent tools to measure the Galactic mass distribution and show promise to probe the nature of dark matter. For successful application of these…

星系天体物理 · 物理学 2026-03-30 Colin Holm-Hansen , Yingtian Chen , Oleg Y. Gnedin

The $\Lambda$CDM cosmological scenario predicts that our Galaxy should contain hundreds of stellar streams at the solar vicinity, fossil relics of the merging history of the Milky Way and more generally of the hierarchical growth of…

星系天体物理 · 物理学 2017-08-23 I. Jean-Baptiste , P. Di Matteo , M. Haywood , A. Gomez , M. Montuori , F. Combes , B. Semelin

We present maps of the stellar streams detected in the Gaia Data Release 2 (DR2) and Early Data Release 3 (EDR3) catalogs using the STREAMFINDER algorithm. We also report the spectroscopic follow-up of the brighter DR2 stream members…

Simulations of tidal streams show that close encounters with dark matter subhalos induce density gaps and distortions in on-sky path along the streams. Accordingly, observing disrupted streams in the Galactic halo would substantiate the…

星系天体物理 · 物理学 2017-07-26 Emily Sandford , Andreas H. W. Kuepper , Kathryn V. Johnston , Juerg Diemand

Mergers and tidal interactions between massive galaxies and their dwarf satellites are a fundamental prediction of the Lambda-Cold Dark Matter cosmology. These events are thought to provide important observational diagnostics of nonlinear…

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