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相关论文: Decoupled gas kinematics in isolated S0 galaxies

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We have studied a sample of completely isolated galaxies by means of long-slit spectroscopy at the 6-m telescope. We have found that 7 of 12 (58 +/- 14 %) galaxies have revealed a presence of large-scale ionized-gas component which angular…

星系天体物理 · 物理学 2014-06-19 Ivan Katkov , Olga Sil'chenko , Victor Afanasiev

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

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

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

We have considered some results concerning gas and stars kinematics of nearby galaxies recently obtained on the SAO RAS 6m telescope using the panoramic spectroscopy methods. The circumnuclear regions of the galaxies were observed with…

天体物理学 · 物理学 2015-06-24 A. V. Moiseev

We review our current knowledge about a particular case of decoupled gas kinematics -- inner ionized-gas polar disks. Though more difficult to be noticed, they seem to be more numerous than their large-scale counterparts; our recent…

星系天体物理 · 物理学 2014-06-19 Olga K. Sil'chenko , Alexei V. Moiseev

(abridged) Photometry and long-slit spectroscopy are presented for a sample of 6 galaxies with a low surface brightness stellar disc and a bulge. The stellar and ionised-gas kinematics were measured along the major and minor axis in half of…

天体物理学 · 物理学 2009-11-13 A. Pizzella , E. M. Corsini , M. Sarzi , J. Magorrian , J. Mendez-Abreu , L. Coccato , L. Morelli , F. Bertola

We present results of our ongoing study of the morphology and kinematics of the ionised gas in 48 representative nearby elliptical and lenticular galaxies using the SAURON integral-field spectrograph on the 4.2m William Herschel Telescope.…

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

Ionized gas and stellar kinematical parameters have been measured along the major axis of 20 nearby disc galaxies. We discuss the properties of each sample galaxy distinguishing between those characterized by regular or peculiar kinematics.…

(Abridged) We present observations of the stellar and gas kinematics for a representative sample of 24 Sa galaxies obtained with our custom-built integral-field spectrograph SAURON operating on the William Herschel Telescope. Our maps…

In a previous study on gas-stellar counterrotation for a large sample of E/S0 and spiral galaxies (Kannappan & Fabricant 2001), two dwarf irregular galaxies were included, of which one was tentatively identified as a counterrotator. Here we…

天体物理学 · 物理学 2008-11-26 J. M. Guie , S. J. Kannappan , Z. Balog , P. Berlind

We analyse the extended, ionized-gas emission of 24 early-type galaxies (ETGs) at $0<z<1$ from the ESO Distant Cluster Survey (EDisCS). We discuss different possible sources of ionization and favour star-formation as the main cause of the…

We present the results of study of the ionized gas velocity fields in 28 nearby (systemic velocity below 1000 km/s) dwarf galaxies. The observations were made at the 6-m BTA telescope of the SAO RAS with the scanning Fabry-Perot…

星系天体物理 · 物理学 2015-06-18 A. V. Moiseev

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

Using various techniques of optical observations at the 6-m Russian telescope (emission-line images, long-slit and 3D spectroscopy), we have studied large-scale morphology and kinematics of the ionized gas in the Seyfert galaxy Mrk6. Having…

星系天体物理 · 物理学 2018-09-26 A. A. Smirnova , A. V. Moiseev , S. N. Dodonov

We present a study of the ionized gas in a sample of 65 nearby early-type galaxies, for which we have acquired optical intermediate-resolution spectra. Emission lines are detected in ~89 % of the sample. The incidence of emission appears…

宇宙学与河外天体物理 · 物理学 2009-09-23 F. Annibali , A. Bressan , R. Rampazzo , W. W. Zeilinger

The origin of the cold gas in central galaxies in groups is still a matter of debate. We present Multi-Unit Spectroscopic Explorer (MUSE) observations of 18 optically selected local Brightest Group Galaxies (BGGs) to study the kinematics…

Misalignments between the rotation axis of stars and gas are an indication of external processes shaping galaxies throughout their evolution. Using observations of 3068 galaxies from the SAMI Galaxy Survey, we compute global kinematic…

The new observational data concerning distribution, excitation, and kinematics of the ionized gas in the giant early-type disk galaxy NGC 2655 obtained at the 6m telescope of the Special Astrophysical Observatory (SAO RAS) and at the 2.5m…

星系天体物理 · 物理学 2023-01-16 Olga K. Sil'chenko , Alexei V. Moiseev , Alexandre S. Gusev , Daria V. Kozlova
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