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Related papers: Seyfert's Sextet: A Slowly Dissolving Stephan's Qu…

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Stephan's Quintet (SQ) is a compact group of galaxies that exhibits numerous signs of interactions between its members. Using high resolution images of SQ in B438, V606, and I814 bands from the Early Release Science project obtained with…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 K. Fedotov , S. C. Gallagher , I. S. Konstantopoulos , R. Chandar , N. Bastian , J. C. Charlton , B. Whitmore , G. Trancho

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…

We present smoothed particle hydrodynamic models of the interactions in the compact galaxy group, Stephan's Quintet. This work is extension of the earlier collisionless N-body simulations of Renaud et al. in which the large-scale stellar…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-30 Jeong-Sun Hwang , Curtis Struck , Florent Renaud , Philip Appleton

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…

This paper is the first of a series addressed to the investigation of galaxy formation/evolution in small scale systems of galaxies (SSSGs) which are located in low density cosmic environments. Our algorithm for SSSG selection includes…

Astrophysics · Physics 2009-11-07 L. Tanvuia , B. Kelm , P. Focardi , R. Rampazzo , W. W. Zeilinger

We present simulations of the compact galaxy group Stephan's Quintet (SQ) including magnetic fields, performed with the N-body/smoothed particle hydrodynamics (SPH) code \textsc{Gadget}. The simulations include radiative cooling, star…

Astrophysics of Galaxies · Physics 2015-06-05 Annette Geng , Alexander M. Beck , Klaus Dolag , Florian Bürzle , Marcus C. Beck , Hanna Kotarba , Peter Nielaba

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…

Astrophysics · Physics 2009-11-06 S. C. Gallagher , J. C. Charlton , S. D. Hunsberger , D. Zaritsky , B. C. Whitmore

The detection of a high velocity (~ 0.3c) inflow of highly ionized matter during an extended XMM-Newton observation of the luminous Seyfert galaxy PG 1211+143 in 2014 provided the first direct evidence of a short-lived accretion event, and…

High Energy Astrophysical Phenomena · Physics 2024-06-11 Ken Pounds , Kim Page

we present the first GALEX UV images of the well known interacting group of galaxies, Stephan's Quintet (SQ). We detect widespread UV emission throughout the group. However, there is no consistent coincidence between UV structure and…

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…

Astrophysics · Physics 2007-05-23 S. C. Gallagher , S. D. Hunsberger , J. C. Charlton , D. Zaritsky

We use smoothed particle hydrodynamics (SPH) models to study the large-scale morphology and dynamical evolution of the intergalactic gas in Stephan's Quintet, and compare to multiwavelength observations. Specifically, we model the formation…

Cosmology and Nongalactic Astrophysics · Physics 2009-08-26 Jeong-Sun Hwang , Curtis Struck , Florent Renaud , Philip N. Appleton

Preliminary results are presented for a spectroscopic survey of the Groth Survey Strip (GSS), a 40 by 3.5 arcminute region of the sky imaged with HST, for which several hundred galaxy spectra have been obtained as part of the DEEP project…

Astrophysics · Physics 2007-05-23 Vicki Sarajedini

The magnitude-limited catalog of the Southern Sky Redshift Survey (SSRS2), is used to characterize the properties of galaxies hosting Active Galactic Nuclei. Using emission-line ratios, we identify a total of 162 (3%) Seyfert galaxies out…

Astrophysics · Physics 2009-11-10 Marcio A. G. Maia , Rodolfo S. Machado , Christopher N. A. Willmer

We present new important results about the intermediate-type Seyfert galaxy Mrk 315, recently observed through optical imaging and integral-field spectroscopy. Broad-band images were used to study the morphology of the host galaxy,…

We present a Gemini-GMOS spectroscopic study of HST-selected H{\alpha}-emitting regions in Stephan's Quintet (HCG 92), a nearby compact galaxy group, with the aim of disentangling the processes of shock-induced heating and star formation in…

We present new spectroscopic observations of 5 galaxies, members of the unusually active compact group HCG 16, observed using the Palomar 5m telescope. The high signal to noise ratios (S/N $\sim 70$) of the spectra allow us to study the…

Astrophysics · Physics 2009-10-31 Reinaldo R. de Carvalho , Roger Coziol

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…

We present results concerning the occurrence of Seyfert galaxies in a new large sample of Compact Groups (Focardi & Kelm 2002). Seyfert galaxies turn out to be relatively rare (<3%), with a significant dominance of Sy2. Seyferts are…

Astrophysics · Physics 2007-05-23 P. Focardi , B. Kelm , V. Zitelli , G. Sarti

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…

We present the first result of a programme to search for large flux variations in the X-ray sources of the XMM Serendipitous Survey compared to previous ROSAT observations. An increase in X-ray flux by a factor >10 was discovered from the…

Astrophysics · Physics 2009-11-10 W. Yuan , St. Komossa , D. Xu , J. P. Osborne , M. G. Watson , R. G. McMahon