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相关论文: Lenticular galaxy IC 719: current building of the …

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The formation scenario of extended counter-rotating stellar disks in galaxies is still debated. In this paper, we study the S0 galaxy IC 719 known to host two large-scale counter-rotating stellar disks in order to investigate their…

We present results of long-slit and panoramic spectroscopy of extended gaseous disks in 18 nearby S0 galaxies, mostly in groups. The gas in our S0s is found to be often accreted from outside that is implied by its decoupled kinematics: at…

星系天体物理 · 物理学 2019-09-11 Olga K. Sil'chenko , Alexei V. Moiseev , Oleg V. Egorov

We used deep long-slit spectra and integral-field spectral data to study the stars and ionized gas kinematics and stellar population properties in the lenticular barred galaxy NGC 7743. We have shown that ionized gas at the distances larger…

宇宙学与河外天体物理 · 物理学 2015-05-28 Ivan Yu. Katkov , Alexei V. Moiseev , Olga K. Sil'chenko

We present the results of the VLT/VIMOS integral-field spectroscopic observations of the inner 28"x28" (3.1 kpc x 3.1 kpc) of the interacting spiral NGC 5719, which is known to host two co-spatial counter-rotating stellar discs. At each…

Lenticular galaxies are generally thought to have descended from spirals via morphological transformation, although recent numerical simulations have shown that minor or even major merger can also lead to an S0-like remnant. These…

星系天体物理 · 物理学 2018-08-08 Kanak Saha , Arianna Cortesi

The nearby S0 galaxy IC 5181 is studied to address the origin of the ionized gas component that orbits the galaxy on polar orbit. We perform detailed photometric and spectroscopic observations measuring the surface brightness distribution…

星系天体物理 · 物理学 2014-04-04 Alessandro Pizzella , Lorenzo Morelli , Enrico Maria Corsini , Elena Dalla Bonta` , Mary Cesetti

We describe the evolution of hot interstellar gas in a family of low luminosity elliptical galaxies all having $M_B = -20$ but with different degrees of flattening (E0, E2, and E6) caused by rotation. The interstellar gas is furnished by…

天体物理学 · 物理学 2009-10-30 Fabrizio Brighenti , William G. Mathews

Chemical abundances in the Leo ring, the largest HI cloud in the local Universe, have recently been determined to be close or above solar, incompatible with a previously claimed primordial origin of the ring. The gas, pre-enriched in a…

星系天体物理 · 物理学 2021-07-21 Edvige Corbelli , Filippo Mannucci , David Thilker , Giovanni Cresci , Giacomo Venturi

By combining new long-slit spectral data obtained with the Southern African Large Telescope (SALT) for 9 galaxies with previously published our observations for additional 12 galaxies we study the stellar and gaseous kinematics as well as…

星系天体物理 · 物理学 2015-05-07 Ivan Yu. Katkov , Alexei Yu. Kniazev , Olga K. Sil'chenko

Rings in S0s are enigmatic features which can however betray the evolutionary paths of particular galaxies. We have undertaken long-slit spectroscopy of five lenticular galaxies with UV-bright outer rings. The observations have been made…

星系天体物理 · 物理学 2019-06-19 Irina S. Proshina , Alexei Yu. Kniazev , Olga K. Sil'chenko

Ionized gas and stellar kinematics have been measured along the major axes of seventeen nearby spiral galaxies of intermediate to late morphological type. We discuss the properties of each sample galaxy distinguishing between those…

天体物理学 · 物理学 2009-11-10 A. Pizzella , E. M. Corsini , J. C. Vega-Beltran , F. Bertola

Galaxies accrete material from the environment through acquisition and merging events. We study the nearby S0 galaxy IC 5181 to address the origin of the ionized-gas component orbiting the galaxy on polar orbit ionized gas of IC 5181 from…

宇宙学与河外天体物理 · 物理学 2015-06-17 Alessandro Pizzella , Lorenzo Morelli , Enrico Maria Corsini , E. Dalla Bontà , Mary Cesetti

In the local (redshift z~0) Universe, collisional ring galaxies make up only ~0.01% of galaxies and are formed by head-on galactic collisions that trigger radially propagating density waves. These striking systems provide key snapshots for…

The oxygen abundance of the outer disk of the nearby S0 galaxy NGC 404, a prototypical early-type galaxy with extended star formation, has been derived from the analysis of HII region spectra. The high mean value found, 12+log(O/H)=8.6 \pm…

宇宙学与河外天体物理 · 物理学 2015-06-16 Fabio Bresolin

The formation pathways of lenticular galaxies (S0s) in field environments remain a matter of debate. We utilize the cosmological hydrodynamic simulation, NewHorizon, to investigate the issue. We select two massive star-formation quenched…

Though S0 galaxies are usually thought to be `red and dead', they demonstrate often star formation organized in ring structures. We try to clarify the nature of this phenomenon and its difference from star formation in spiral galaxies. The…

星系天体物理 · 物理学 2020-02-19 I. Proshina , O. Sil'chenko , A. Moiseev

We report a discovery of extended counterrotating gaseous disks in early-type disk galaxies NGC 2551 and NGC 5631. To find them, we have undertaken complex spectral observations including integral-field spectroscopy for the central parts of…

天体物理学 · 物理学 2011-02-11 O. K. Sil'chenko , A. V. Moiseev , V. L. Afanasiev

Lenticular galaxies remain remarkably mysterious as a class. Observations to date have not led to any broad consensus about their origins, properties and evolution, though they are often thought to have formed in one big burst of star…

天体物理学 · 物理学 2009-11-07 Gary A. Welch , Leslie J. Sage

A sample of completely isolated S0 galaxies has been studied by means of long-slit spectroscopy at the Russian 6-m telescope. 7 of 12 galaxies have revealed a presence of extended ionized-gas discs which rotation is mostly decoupled from…

星系天体物理 · 物理学 2015-06-18 Ivan Katkov , Olga Sil'chenko , Victor Afanasiev

We present interferometric HI observations of six double-disc stellar counterrotator ("2$\sigma$") galaxies from the Atlas3D sample. Three are detected in HI emission; two of these are new detections. NGC 7710 shows a modestly asymmetric HI…

星系天体物理 · 物理学 2020-05-13 Lisa M Young , Davor Krajnović , Pierre-Alain Duc , Paolo Serra
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