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相关论文: IC 5181: An S0 Galaxy with Ionized Gas on Polar Or…

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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

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 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 present new observations of the [Ne II] emission from the ionized gas in Sgr A West with improved resolution and sensitivity. About half of the emission comes from gas with kinematics indicating it is orbiting in a plane tipped about…

星系天体物理 · 物理学 2015-06-05 Wesley T. Irons , John H. Lacy , Matthew J. Richter

I review the current understanding of the origin and nature of ``warm'' ionized gas in giant elliptical galaxies in the light of results of recent imaging and spectroscopic surveys. CCD imaging surveys have revealed that emission-line disks…

天体物理学 · 物理学 2007-05-23 Paul Goudfrooij

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

We present results from an on-going programme to study the dust and ionized gas in E/S0 galaxies with dust lanes. Our data, together with results from previous studies of E/S0 galaxies, are used to demonstrate the tight relationship between…

宇宙学与河外天体物理 · 物理学 2015-06-04 Ido Finkelman , Noah Brosch , S. J. Jose G. Funes , Sudhanshu Barway , Alexei Kniazev , Petri Vaisanen

We have obtained and analyzed long-slit spectral data for the lenticular galaxy IC 719. In this gas-rich S0 galaxy, its large-scale gaseous disk counterrotates the global stellar disk. Moreover in the IC 719 disk we have detected a…

宇宙学与河外天体物理 · 物理学 2013-05-14 Ivan Yu. Katkov , Olga K. Sil'chenko , Victor L. Afanasiev

IC 1459 is an early-type galaxy (ETG) with a rapidly counter-rotating stellar core, and is the central galaxy in a gas-rich group of spirals. In this work, we investigate the abundant ionized gas in IC 1459 and present new stellar orbital…

星系天体物理 · 物理学 2021-04-28 Celia R. Mulcahey , Laura J. Prichard , Davor Krajnovic , Regina A. Jorgenson

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

Our objective is to investigate the physical properties of the ionised gas of the low-metallicity dwarf galaxy, IC 10, at various spatial scales: from individual HII regions to the entire galaxy scale and examine whether diagnostics for…

The nearby dwarf galaxy NGC 3077 is known for its peculiar morphology, which includes numerous dust lanes and emission-line regions. The interstellar medium in this galaxy is subject to several perturbing factors. These are primarily the…

星系天体物理 · 物理学 2021-01-20 D. V. Oparin , O. V. Egorov , A. V. Moiseev

IC 10 is the nearest starburst irregular galaxy remarkable for its anomalously high number of WR stars. We report the results of an analysis of the emission spectra of HII-regions ionized by star clusters and WR stars based on observations…

宇宙学与河外天体物理 · 物理学 2015-05-19 O. V. Egorov , V. P. Arkhipova , T. A. Lozinskaya , A. V. Moiseev

Galactic circumnuclear environments of nearby galaxies provide unique opportunities for our understanding of the co-evolution between super-massive black holes and their host galaxies. Here we present a detailed study of ionized gas in the…

星系天体物理 · 物理学 2022-04-06 Zongnan Li , Zhiyuan Li , Ruben Garcia-Benito , Shuai Feng

We report the results of multicolour observations of 30 E/S0 galaxies with dust lanes. For each galaxy we obtained broad-band images and narrow-band images using interference filters isolating the H\alpha +[NII] emission lines to derive the…

宇宙学与河外天体物理 · 物理学 2015-05-19 Ido Finkelman , Noah Brosch , José G. Funes S. J. , Alexei Y. Kniazev , Petri Väisänen

In this work we investigate the stellar population, metallicity distribution and ionized gas in the elliptical galaxy NGC 5044, using long-slit spectroscopy and a stellar population synthesis method. We found differences in the slope of…

天体物理学 · 物理学 2007-11-29 M. G. Rickes , M. G. Pastoriza , Ch Bonatto

We present the results of a multiwavelength study of the nearby dwarf galaxy DDO 53 - a relatively isolated member of the M 81 group. We analyse the atomic and ionised gas kinematics (based on the observations with Fabry-Perot…

We present the results of observations of the Irr galaxy IC 10 at the 6-m SAO telescope with the panoramic Multi-Pupil Fiber Spectrograph (MPFS). Based on the results of these observations and our long-slit spectroscopy performed…

宇宙学与河外天体物理 · 物理学 2011-07-15 V. P. Arkhipova , O. V. Egorov , T. A. Lozinskaya , A. V. Moiseev

We performed an integrated optical polarization survey of 70 nearby galaxies to study the relationship between linear polarization and galaxy properties. To date this is the largest survey of its kind. The data were collected at McDonald…

宇宙学与河外天体物理 · 物理学 2015-06-03 Amy Jones , Lifan Wang , Kevin Krisciunas , Emily Freeland

In early type galaxies, externally accreted gas is thought to be the main source of gas replenishment at late times. We use MUSE integral field spectroscopy data to study the active S0 galaxy NGC 5077, known to have disturbed dynamics,…

星系天体物理 · 物理学 2021-06-09 Sandra I. Raimundo
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