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Tidal interaction governs the redistribution of angular momentum in close binary stars and planetary systems and determines the systems evolution towards the possible equilibrium state. Turbulent friction acting on the equilibrium tide in…

太阳与恒星天体物理 · 物理学 2018-07-11 P. G. Beck , S. Mathis , F. Gallet , C. Charbonnel , M. Benbakoura , R. A. García , J. -D. do Nascimento

The introduction of thermodynamics into gravitational physics began 5 decades ago with the discovery that black holes behave like thermodynamic systems once semiclassical quantum effects are taken into account. Notions of temperature,…

广义相对论与量子宇宙学 · 物理学 2025-08-05 Robert B. Mann

We review results on the dynamics of warped gaseous discs. We consider tidal perturbation of a Keplerian disc by a companion star orbiting in a plane inclined to the disc. The perturbation induces the precession of the disc, and thus of any…

天体物理学 · 物理学 2007-05-23 C. Terquem , J. Papaloizou , R. Nelson

The galactic evolutionary theory is now sufficiently mature to provide information about the galaxy formation phase. From evolutionary models we establish a link between the present features of late type galaxies and the protogalactic…

天体物理学 · 物理学 2011-04-15 Claudio Firmani , Xavier Hernández , Vladimir Avila-Reese

We present a semi-analytical model in which galaxy collisions and strong tidal interactions, both in the field and during the collapse phase of groups and clusters help determine galaxy morphology. From a semi-analytical analysis based on…

天体物理学 · 物理学 2009-10-30 C. Balland , J. Silk , R. Schaeffer

Observations of massive stars within the central parsec of the Galaxy show that, while most stars orbit within a well-defined disc, a significant fraction have large eccentricities and / or inclinations with respect to the disc plane. Here,…

天体物理学 · 物理学 2009-03-08 Jorge Cuadra , Philip J. Armitage , Richard D. Alexander

While gas accretion onto some massive black holes (MBHs) at the centers of galaxies actively powers luminous emission, the vast majority of MBHs are considered dormant. Occasionally, a star passing too near a MBH is torn apart by…

In this paper, we want to study the tidal effect of an external perturber upon a disc galaxy based on the generalization of already used Keplerian potential. The generalization of the simple ideal Keplerian potential includes an orbital…

综合物理 · 物理学 2015-11-09 M. Alavi , H. Razmi

Supermassive disks are thought to be precursors of supermassive black holes that are believed to power quasars and exist at centers of galaxies. Formation scenarios of such disks are reviewed and it is argued that gas dynamical schemes are…

天体物理学 · 物理学 2007-05-23 A. Mangalam

The Galactic Center has been under intense scrutiny in the recent years thanks to the unprecedented missions aiming at measuring the gas and star dynamics near the supermassive black hole (SMBH) and at finding gravitational wave (GW)…

星系天体物理 · 物理学 2019-11-13 Re'em Sari , Giacomo Fragione

Space-based time-domain telescopes such as CoRoT, Kepler/K2 and TESS have profoundly impacted astrophysics over the past two decades. Continuous light curves with high cadence and high photometric precision are now available for millions of…

太阳与恒星天体物理 · 物理学 2025-12-12 Daniel Huber

Recent spectroscopic observations of galaxies in distant clusters have revealed that the rate of star formation in star-forming galaxies is significantly suppressed with respect to their counterparts in the field at a similar redshift. It…

天体物理学 · 物理学 2015-06-24 Kenji Bekki , Warrick J. Couch , Yasuhiro Shioya

We report the serendipitous discovery of a bright point source flare in the Abell cluster 1795 with archival EUVE and Chandra observations. Assuming the EUVE emission is associated with the Chandra source, the X-ray 0.5-7 keV flux declined…

The equilibrium state of a turbulent clumpy gas disk is analytically investigated. The disk consists of distinct self-gravitating clouds. Gravitational cloud-cloud interactions transfer energy over spatial scales and produce a viscosity,…

天体物理学 · 物理学 2009-11-07 B. Vollmer , T. Beckert

We consider formation of accretion disks from a realistically turbulent molecular gas using 3D MHD simulations. In particular, we analyze the effect of the fast turbulent reconnection described by the Lazarian & Vishniac (1999) model for…

太阳与恒星天体物理 · 物理学 2016-03-16 Diego F. González-Casanova , Reinaldo Santos-Lima , Alexander Lazarian

We study the joint effect of tidal torques and dynamical friction on the collapse of density peaks solving numerically the equations of motion of a shell of barionic matter falling into the central regions of a cluster of galaxies. We…

天体物理学 · 物理学 2007-05-23 A. Del Popolo , M. Gambera

Tidal disruption events\,(TDEs) provide a valuable probe in studying the dynamics of stars in the nuclear environments of galaxies. Recent observations show that TDEs are strongly overrepresented in post-starburst or "green valley"…

高能天体物理现象 · 物理学 2024-01-01 Mengye Wang , Yiqiu Ma , Qingwen Wu , Ning Jiang

The theory for the selection of the initial state of the universe from the landscape multiverse predicts superhorizon inhomogeneities induced by nonlocal entanglement of our Hubble volume with modes and domains beyond the horizon. Here we…

高能物理 - 理论 · 物理学 2009-02-09 L. Mersini-Houghton , R. Holman

Nikos Voglis had many astronomical interests, among them was the question of the origin of galactic angular momentum. In this short tribute we review how this subject has changed since the 1970's and how it has now become evident that…

天体物理学 · 物理学 2015-05-13 Bernard J. T. Jones , Rien van de Weygaert

Extended, soft X-ray emission from the halo of a very large disk galaxy has been detected out to r~20-40 kpc. The luminosity and surface brightness distribution is in very good agreement with predictions by recent, cosmological galaxy…

天体物理学 · 物理学 2015-06-24 Jesper Sommer-Larsen