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We use deep imaging from the Dark Energy Camera to explore the peripheral regions of nine globular clusters in the outer halo of the Milky Way. Apart from Whiting 1 and NGC 7492, which are projected against the Sagittarius stream, we see no…

星系天体物理 · 物理学 2022-03-30 Shumeng Zhang , Dougal Mackey , Gary Da Costa

Stellar streams are sensitive probes of the Milky Way's gravitational potential. The mean track of a stream constrains global properties of the potential, while its fine-grained surface density constrains galactic substructure. A precise…

STREAMFINDER is a new algorithm that we have built to detect stellar streams in an automated and systematic way in astrophysical datasets that possess any combination of positional and kinematic information. In Paper I, we introduced the…

The peripheral regions of globular clusters (GCs) are extremely challenging to study due to their low surface brightness nature and the dominance of Milky Way contaminant populations along their sightlines. We have developed a probabilistic…

星系天体物理 · 物理学 2021-08-18 Pete B. Kuzma , Annette M. N. Ferguson , Jorge Peñarrubia

[Abridged] Within the hierarchical framework for galaxy formation, minor merging and tidal interactions are expected to shape all large galaxies to the present day. As a consequence, most seemingly normal disk galaxies should be surrounded…

We present a new method for determining the Galactic gravitational potential based on forward modeling of tidal stellar streams. We use this method to test the performance of smooth and static analytic potentials in representing realistic…

星系天体物理 · 物理学 2015-06-22 Ana Bonaca , Marla Geha , Andreas H. W. Kuepper , Juerg Diemand , Kathryn V. Johnston , David W. Hogg

Extended halo tidal streams from disrupting Milky Way satellites offer new opportunities for gauging fundamental Galactic parameters without challenging observations of the Galactic center. In the roughly spherical Galactic potential tidal…

天体物理学 · 物理学 2009-11-13 Steven R. Majewski , David R. Law , Allyson A. Polak , Richard J. Patterson

The Sagittarius stream is one of the best tools that we currently have to estimate the mass and shape of our Galaxy. However, assigning membership and obtaining the phase-space distribution of the stars that form the tails is quite…

星系天体物理 · 物理学 2020-07-27 P. Ramos , C. Mateu , T. Antoja , A. Helmi , A. Castro-Ginard , E. Balbinot , J. M. Carrasco

Recent analysis of the second data release of Gaia has revealed a number of new stellar streams surrounding the Milky Way. It has been suggested that one of these streams, Gj\"oll, is associated with the globular cluster NGC 3201, but thus…

太阳与恒星天体物理 · 物理学 2021-09-01 T. T. Hansen , A. H. Riley , L. E. Strigari , J. L. Marshall , P. S. Ferguson , J. Zepeda , C. Sneden

In the hierarchical formation scenario in which the outer halo of the Milky Way is the result of the continuous accretion of low-mass galaxies, a fraction of the Galactic globular cluster system might have originated in and been accreted…

We present results on the extra-tidal features of the Milky Way globular cluster NGC 7099, using deep gr photometry obtained with the Dark Energy Camera (DECam). We reached nearly 6 mag below the cluster Main Sequence (MS) turnoff, so that…

星系天体物理 · 物理学 2020-10-28 A. E. Piatti , J. A. Carballo-Bello , M. D. Mora , C. Cenzano , C. Navarrete , M. Catelan

We present SkyCURTAINs, a data driven and model agnostic method to search for stellar streams in the Milky Way galaxy using data from the Gaia telescope. SkyCURTAINs is a weakly supervised machine learning algorithm that builds a background…

星系天体物理 · 物理学 2024-05-22 Debajyoti Sengupta , Stephen Mulligan , David Shih , John Andrew Raine , Tobias Golling

One of the most promising tracers of the Galactic potential in the halo region are stellar streams. However, individual stream fits can be limited by systematic biases. To study these individual stream systematics, we fit streams in Milky…

星系天体物理 · 物理学 2021-11-17 Stella Reino , Robyn E. Sanderson , Nondh Panithanpaisal , Elena M. Rossi , Konrad Kuijken

We discuss how to use tidal streams from globular clusters to measure the mass distribution of the Milky Way. Recent proper motion determinations for globular clusters from plate measurements and Hipparcos astrometry provide several good…

天体物理学 · 物理学 2009-10-31 C. Murali , J. Dubinski

We report the result of searching for globular clusters (GCs) around 55 Milky Way satellite dwarf galaxies within the distance of 450 kpc from the Galactic Center except for the Large and Small Magellanic Clouds and the Sagittarius dwarf.…

星系天体物理 · 物理学 2020-11-04 Kuan-Wei Huang , Sergey E. Koposov

Stellar streams produced from dwarf galaxies provide direct evidence of the hierarchical formation of the Milky Way. Here, we present the first comprehensive study of the "LMS-1" stellar stream, that we detect by searching for wide streams…

星系天体物理 · 物理学 2021-10-20 Khyati Malhan , Zhen Yuan , Rodrigo Ibata , Anke Arentsen , Michele Bellazzini , Nicolas F. Martin

Tidal features from galaxy mergers, particularly stellar streams, offer valuable insights into galaxy assembly and dark matter halo properties. This paper aims to identify a large sample of nearby stellar streams suitable for detailed…

An all high-latitude sky survey for cool carbon giant stars in the Galactic halo has revealed 75 such stars, of which the majority are new detections. Of these, more than half are clustered on a Great Circle on the sky which intersects the…

天体物理学 · 物理学 2009-10-31 Rodrigo Ibata , Geraint F. Lewis , Michael Irwin , Edward Totten , Thomas Quinn

Using photometry and proper motions from Pan-STARRS, DECaLS, and Gaia DR3, we detect a ~35 to 70 degree-long trailing stellar debris stream associated with the globular cluster NGC 288. The trajectory of the trailing tail is not well…

星系天体物理 · 物理学 2024-12-31 Carl J. Grillmair