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相关论文: The Shape and Orientation of NGC 3379: Implication…

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We present the results from a detailed kinematic analysis of both ground-based, and Hubble Space Telescope/Faint Object Camera long-slit spectroscopy at sub-arcsec spatial resolution, of the narrow-line region of NGC 4151. In agreement with…

天体物理学 · 物理学 2009-10-31 Claudia Winge , David J. Axon , F. D. Macchetto , A. Capetti , A. Marconi

The superimposed pair of spiral galaxies NGC 3314 offers a unique opportunity to trace the dust properties in a spiral galaxy. We analyze multicolor HST imaging, supported by ground-based near-IR imaging and fiber-array spectroscopy to…

天体物理学 · 物理学 2009-11-06 William C. Keel , Raymond E. White

We analyse VLT/MUSE observations of PGC 046832, the brightest cluster galaxy of Abell 3556. The velocity structure of this galaxy is startling and shows two reversals in sign along the minor axis, and one along the major axis. We use…

星系天体物理 · 物理学 2021-10-13 Mark den Brok , Davor Krajnović , Eric Emsellem , Jarle Brinchmann , Michael Maseda

Several thousand solar masses of molecular, atomic and ionized gas lie in the innermost ~10 pc of our Galaxy. The most relevant structure of molecular gas is the circumnuclear ring (CNR), a dense and clumpy ring surrounding the supermassive…

星系天体物理 · 物理学 2016-01-20 Michela Mapelli , Alessandro A. Trani

Observations with the Hubble Space Telescope reveal an irregular network of dust spiral arms in the nuclear region of the interacting disk galaxy NGC 2207. The spirals extend from ~50 pc to ~300 pc in galactocentric radius, with a projected…

天体物理学 · 物理学 2015-06-24 B. G. Elmegreen , D. M. Elmegreen , E. Brinks , C. Yuan , M. Kaufman , M. Klaric , L. Montenegro , C. Struck , M. Thomasson

We present analysis of the three-dimensional shape of intracluster gas in clusters formed in cosmological simulations of the Lambda-CDM cosmology and compare it to the shape of dark matter distribution and the shape of the overall…

宇宙学与河外天体物理 · 物理学 2015-05-18 Erwin T. Lau , Daisuke Nagai , Andrey V. Kravtsov , Andrew R. Zentner

We present a harmonic expansion of the observed line-of-sight velocity field as a method to recover and investigate spiral structures in the nuclear regions of galaxies. We apply it to the emission-line velocity field within the…

星系天体物理 · 物理学 2010-12-27 Glenn van de Ven , Kambiz Fathi

We present $B,V,R,J,H,K$ broad--band images of the barred galaxy NGC 1097. The optical and infrared colors maps trace the location of the major dust features. The dust lanes are relatively free of star formation and have low opacity. The…

天体物理学 · 物理学 2009-10-28 A. C. Quillen , Jay. A. Frogel , L. E. Kuchinski , D. M. Terndrup

We present a high-resolution (R~16,000) spectrum and a narrow-band image centered on the [NeII]12.8 micron line of the central kpc region of the starburst/Seyfert2 galaxy NGC 7582. The galaxy has a rotating circum-nuclear starburst disk,…

天体物理学 · 物理学 2009-11-11 M. Wold , M. Lacy , H. U. Kaeufl , R. Siebenmorgen

The consequences of nuclear black holes for the structure and dynamics of stellar spheroids are reviewed. Slow growth of a black hole in a pre-existing core produces a steep power-law density profile similar to the cusps seen in faint…

天体物理学 · 物理学 2007-05-23 David Merritt

SRG/eROSITA PV observations revealed the A3391/95 cluster system and the Northern Clump (MCXC J0621.7-5242 galaxy cluster) are aligning along a cosmic filament in soft X-rays, similarly to what has been seen in simulations before. We aim to…

We present HST STIS observations of the galaxy NGC 4382 (M85) and axisymmetric models of the galaxy to determine mass-to-light ration (M/L, V-band) and central black hole mass (M_BH). We find M/L = 3.74 +/- 0.1 (solar units) and M_BH = 1.3…

宇宙学与河外天体物理 · 物理学 2015-05-30 Kayhan Gultekin , Douglas O. Richstone , Karl Gebhardt , S. M. Faber , Tod R. Lauer , Ralf Bender , John Kormendy , Jason Pinkney

We present Gemini/GNIRS spectroscopy of the Seyfert 2 galaxy NGC 4388, with simultaneous coverage from 0.85 - 2.5 $\mu$m. Several spatially-extended emission lines are detected for the first time, both in the obscured and unobscured portion…

We present a unique set of nested stellar kinematical maps of NGC 3377 obtained with the integral-field spectrographs OASIS and SAURON. We then construct general axisymmetric dynamical models for this galaxy, based on the Schwarzschild…

天体物理学 · 物理学 2007-05-23 Y. Copin , N. Cretton , E. Emsellem

We have analysed a new high-resolution e-MERLIN 1.5 GHz radio continuum map together with $HST$ and SDSS imaging of NGC 5322, an elliptical galaxy hosting radio jets, aiming to understand the galaxy's central structure and its connection to…

We homogeneously measured the elliptical shapes of 163 globular clusters (GCs) using the on-sky distribution of their cluster members and the third data release of the ESA mission Gaia (DR3). The astrometry enables the differentiation of…

星系天体物理 · 物理学 2024-08-02 Mauricio Cruz Reyes , Richard I. Anderson

NGC 3621 is a late-type (Sd) spiral galaxy with an active nucleus, previously detected through mid-infrared [Ne V] line emission. Archival Hubble Space Telescope (HST) images reveal that the galaxy contains a bright and compact nuclear star…

天体物理学 · 物理学 2008-12-18 A. J. Barth , L. E. Strigari , M. C. Bentz , J. E. Greene , L. C. Ho

Recent progress is summarized on the determination of the density distributions of stars and dark matter, stellar kinematics, and stellar population properties, in the extended, low surface brightness halo regions of elliptical galaxies.…

星系天体物理 · 物理学 2015-05-20 Ortwin Gerhard

The non-linear dynamics of bending instability and vertical structure of a galactic stellar disc embedded into a spherical halo are studied with N-body numerical modelling. Development of the bending instability in stellar galactic disc is…

宇宙学与河外天体物理 · 物理学 2015-05-19 A. Khoperskov , D. Bizyaev , N. Tiurina , M. Butenko

We examine the nuclear morphology, kinematics, and stellar populations in nearby S0 galaxy NGC 404 using a combination of adaptive optics assisted near-IR integral-field spectroscopy, optical spectroscopy, and HST imaging. These…