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相关论文: Interpretation of the Stephan Quintet Galaxy Clust…

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Stephan's Quintet (SQ) is a compact group of galaxies that has been well studied since its discovery in 1877 but is mysterious using cold dark matter hierarchical clustering cosmology (CDMHCC). Anomalous red shifts z = (0.0027,0.019, 0.022,…

天体物理学 · 物理学 2007-05-23 Carl H. Gibson , Rudolph E. Schild

Stephan's Quintet (SQ), discovered more than 100 years ago, is the most famous and well studied compact galaxy group. It has been observed in almost all wavebands, with the most advanced instruments including Spitzer, GALEX, HST, Chandra,…

天体物理学 · 物理学 2007-05-23 C. Kevin Xu

Stephan's Quintet (SQ) is a system consisting of at least four interacting galaxies which is well known for its complex dynamical and star formation history. It possesses a rich intergalactic medium (IGM), where hydrogen clouds, both atomic…

Stephan's Quintet (SQ, distance=85$\pm$6 Mpc) is unique among compact groups of galaxies. Observations have previously shown that interactions between multiple members, including a high-speed intruder galaxy currently colliding into the…

星系天体物理 · 物理学 2022-08-11 C. K. Xu , C. Cheng , P. N. Appleton , P. -A. Duc , Y. Gao , N. -Y. Tang , M. Yun , Y. S. Dai , J. -S. Huang , U. Lisenfeld , F. Renaud

Multiwavelength data for Stephan's Quintet (SQ) are consistent with the following model for this compact galaxy group. (1) Discordant redshift NGC 7320 is an unrelated foreground galaxy. (2) In the past SQ was an accordant redshift quartet…

天体物理学 · 物理学 2009-10-30 M. Moles , J. W. Sulentic , I. Márquez

We present HST WFPC2 images of Stephan's Quintet which encompass three interacting galaxies and their associated tidal features. These deep, three-color (B, V, I) images indicate recent, massive stellar system formation in various regions…

天体物理学 · 物理学 2007-05-23 S. C. Gallagher , S. D. Hunsberger , J. C. Charlton , D. Zaritsky

Stephan's Quintet (SQ) is a compact group that we find in an atypical moment when a high velocity intruder is passing through it. The intrusion is particularly interesting because a previous intruder had stripped most of the gas from the…

天体物理学 · 物理学 2009-11-07 Jack W. Sulentic , M. Rosado , D. Dultzin-Hacyan , L. Verdes-Montenegro , G. Trinchieri , C. Xu , W. Pietsch

Stephan's Quintet (SQ) is a Hickson Compact Group well known for its complex dynamical and star formation history and its rich intergalactic medium (IGM). In order to study the extent, origin and fate of the intergalactic molecular gas and…

Stephan's Quintet (SQ) is a local compact galaxy group system that exhibits significant star formation activity. A history of tidal interactions between its four member galaxies and a recent collision between an intruder galaxy and the…

The evolution of compact groups of galaxies may represent one of the few places in the nearby universe in which massive galaxies are being forged through a complex set of processes involving tidal interaction, ram-pressure stripping, and…

宇宙学与河外天体物理 · 物理学 2015-05-19 Florent Renaud , Philip N. Appleton , C. Kevin Xu

Analysis of Hubble Space Telescope/Wide Field Planetary Camera 2 images of Stephan's Quintet, Hickson Compact Group 92, yielded 115 candidate star clusters (with V-I < 1.5). Unlike in merger remants, the cluster candidates in Stephan's…

天体物理学 · 物理学 2009-11-06 S. C. Gallagher , J. C. Charlton , S. D. Hunsberger , D. Zaritsky , B. C. Whitmore

We carried out deep mapping observations of the atomic hydrogen (HI) 21 cm line emission in a field centered on the famous galaxy group Stephan's Quintet (SQ), using the Five-hundred-meter Aperture Spherical Telescope (FAST) equipped with…

Stephan's Quintet, a compact group of galaxies, is often used as a laboratory to study a number of phenomena, including physical processes in the interstellar medium, star formation, galaxy evolution, and the formation of fossil groups. As…

星系天体物理 · 物理学 2018-01-24 Pierre-Alain Duc , Jean-Charles Cuillandre , Florent Renaud

Stephan's Quintet (SQ) is a nearby compact galaxy group and a perfect laboratory for studying the process of galaxy evolution through galaxy harassment and interaction. By analysing the kinematics of SQ we aim to provide an increased…

星系天体物理 · 物理学 2021-12-11 M. Yttergren , P. Misquitta , Á. Sánchez-Monge , M. Valencia-S , A. Eckart , A. Zensus , T. Peitl-Thiesen

Nearby Compact Groups of Galaxies (CGs) are very complex systems, tracing their history is a challenge (e.g. Stephan's Quintet). The presence of a diffuse X-rays emission that often peaks in the center of CGs shows that CGs are bound…

天体物理学 · 物理学 2007-05-23 Philippe Amram , Chantal Balkowski , Claudia Mendes de Oliveira , Henri Plana , Benoit Epinat

Stephan's Quintet (SQ), the prototypical compact group of galaxies in the local Universe, has been observed with the imaging Fourier transform spectrometer SITELLE, attached to the CFHT, to perform a deep search for intergalactic…

星系天体物理 · 物理学 2019-09-13 S. Duarte Puertas , J. Iglesias-Páramo , J. M. Vilchez , L. Drissen , C. Kehrig , T. Martin

Self-gravitational structure formation theory for astrophysics and cosmology is revised using nonlinear fluid mechanics. Gibson's 1996-2000 theory balances fluid mechanical forces with gravitational forces and density diffusion with…

天体物理学 · 物理学 2007-05-23 Carl H. Gibson

Recent observations of Stephan's Quintet gave new indications on its formation scenario. Older formation and a role of NCG 7317 should be considered in revised numerical models of the compact group. Velocities of group members to recreate…

广义相对论与量子宇宙学 · 物理学 2020-03-17 M. L. Abdelali , N. Mebarki

We present new observational evidence supporting the hypothesis that SQ-A, a starburst in the intra-group medium (IGrM) of Stephan's Quintet (SQ), is triggered by a high-speed collision between two gas systems, one associated with the IGrM…

Self-gravitational fluid mechanical methods termed hydro-gravitational-dynamics (HGD) predict plasma fragmentation 0.03 Myr after the turbulent big bang to form protosuperclustervoids, turbulent protosuperclusters, and protogalaxies at the…

天体物理学 · 物理学 2008-08-26 Carl H. Gibson , Rudolph E. Schild
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