中文
相关论文

相关论文: Transient axion streams from disrupted minicluster…

200 篇论文

We present a study of the effects of collisional dynamics on the formation and detectability of cold tidal streams. A semi-analytical model for the evolution of the stellar mass function was implemented and coupled to a fast stellar stream…

星系天体物理 · 物理学 2017-10-24 Eduardo Balbinot , Mark Gieles

We consider misaligned accretion discs formed after tidal disruption events occurring when a star encounters a supermassive rotating black hole. We use the linear theory of warped accretion discs to find the disc shape when the stream…

高能天体物理现象 · 物理学 2018-09-19 P. B. Ivanov , V. V. Zhuravlev , J. C. B. Papaloizou

The tidal disruption of a star by a supermassive black hole provides us with a rare glimpse of these otherwise dormant beasts. It has long been predicted that the disruption will be accompanied by a thermal `flare', powered by the accretion…

高能天体物理现象 · 物理学 2015-05-27 Dimitrios Giannios , Brian D. Metzger

In this paper we discuss a method for the generation of mock tidal streams. Using an ensemble of simulations in an isochrone potential where the actions and frequencies are known, we derive an empirical recipe for the evolving satellite…

星系天体物理 · 物理学 2015-07-15 Mark A. Fardal , Shuiyao Huang , Martin D. Weinberg

Hundreds of globular clusters and dwarf galaxies encircle the Milky Way. Many of these systems have undergone partial disruption due to tidal forces, littering the halo with stellar streams. These tidal tails are sensitive to the Galactic…

太阳与恒星天体物理 · 物理学 2016-08-03 Andrew R. Casey

We estimate collapse rates of axion stars in our galaxy based on the axion minicluster mass function of the Milky Way dark matter halo. We consider axion-like particles with different temperature evolution of the axion mass, including the…

高能物理 - 唯象学 · 物理学 2024-10-18 Dennis Maseizik , Joshua Eby , Hyeonseok Seong , Günter Sigl

The massive galaxies in the young universe, ten billion years ago, formed stars at surprising intensities. Although this is commonly attributed to violent mergers, the properties of many of these galaxies are incompatible with such events,…

天体物理学 · 物理学 2009-11-13 A. Dekel , Y. Birnboim , G. Engel , J. Freundlich , T. Goerdt , M. Mumcuoglu , E. Neistein , C. Pichon , R. Teyssier , E. Zinger

Stellar streams result from the tidal disruption of satellites and star clusters as they orbit a host galaxy, and can be very sensitive probes of the gravitational potential of the host system. We select and study narrow stellar streams…

星系天体物理 · 物理学 2017-03-08 Robyn E. Sanderson , Johanna Hartke , Amina Helmi

Observations of the lengthy tidal streams produced by the destruction of the Sagittarius dwarf spheroidal (Sgr dSph) are capable of providing strong constraints on the shape of the Galactic gravitational potential. However, previous work,…

星系天体物理 · 物理学 2015-05-14 David R. Law , Steven R. Majewski , Kathryn V. Johnston

We develop a framework for modelling the Milky Way using stellar streams and a wide range of photometric and kinematic observations. Through the use of mock data we demonstrate that a standard suite of Galactic observations leads to…

星系天体物理 · 物理学 2014-03-05 Nathan Deg , Lawrence Widrow

Tidal streams of disrupting dwarf galaxies orbiting around their host galaxy offer a unique way to constrain the shape of galactic gravitational potentials. Such streams can be used as leaning tower gravitational experiments on galactic…

星系天体物理 · 物理学 2017-07-12 Guillaume F. Thomas , Benoit Famaey , Rodrigo Ibata , Fabian Lueghausen , Pavel Kroupa

We present a phenomenological description of the properties of tidal tails forming around dwarf galaxies orbiting the Milky Way. For this purpose we use collisionless N-body simulations of dwarfs initially composed of a disk embedded in an…

星系天体物理 · 物理学 2015-10-12 Ewa L. Lokas , Grzegorz Gajda , Stelios Kazantzidis

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…

The dynamics of stellar streams in rotating barred potentials is explained for the first time. Naturally, neighbouring stream stars reach pericentre at slightly different times. In the presence of a rotating bar, these neighbouring stream…

星系天体物理 · 物理学 2018-11-02 Kohei Hattori , Denis Erkal , Jason L. Sanders

Eccentric white dwarf-massive black hole binaries can potentially source some extreme X-ray transients, including the recently observed quasi-periodic X-ray eruptions and tidal disruption events at the galactic nuclei. Meanwhile, they are…

高能天体物理现象 · 物理学 2025-11-13 Shu Yan Lau , Hang Yu

A fundamental prediction of the Lambda Cold Dark Matter (LCDM) cosmology is the centrally divergent cuspy density profile of dark matter haloes. Density cusps render CDM haloes resilient to tides, and protect dwarf galaxies embedded in them…

星系天体物理 · 物理学 2024-06-14 Raphaël Errani , Rodrigo Ibata , Julio F. Navarro , Jorge Peñarrubia , Matthew G. Walker

We present evidence for a new Milky Way stellar tidal stream in the direction of the Andromeda and Triangulum (M31 and M33) galaxies. Using a matched-filter technique, we search the Sloan Digital Sky Survey Data Release 8 by creating…

星系天体物理 · 物理学 2015-06-11 Ana Bonaca , Marla Geha , Nitya Kallivayalil

We present an extragalactic perspective of an extended stellar tidal stream wrapping around the edge-on, spiral galaxy NGC 5907. Our deep images reveal for the first time a large scale complex of arcing loops that is an excellent example of…

According to the current galaxy formation paradigm, mergers and interactions play an important role in shaping present-day galaxies. The remnants of this merger activity can be used to constrain galaxy formation models. In this work we use…

Context. Models of hierarchical structure formation predict the accretion of smaller satellite galaxies onto more massive systems and this process should be accompanied by a disintegration of the smaller companions visible, e.g., in tidal…

星系天体物理 · 物理学 2015-05-27 Arpad Miskolczi , Dominik J. Bomans , Ralf-Jürgen Dettmar