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相关论文: Inner Polar Rings and Disks: Observed Properties

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We have considered polar ring galaxy candidates, the images of which can be found in the SDSS. The sample of 78 galaxies includes the most reliable candidates from the SPRC and PRC catalogs, some of which already have kinematic…

星系天体物理 · 物理学 2015-06-17 K. I. Smirnova , A. V. Moiseev

Based on SDSS data, we have selected a sample of nine edge-on spiral galaxies with bulges whose major axes show a high inclination to the disk plane. Such objects are called polar-bulge galaxies. They are similar in their morphology to…

星系天体物理 · 物理学 2016-01-20 V. P. Reshetnikov , S. S. Savchenko , A. V. Mosenkov , N. Ya. Sotnikova , D. V. Bizyaev

A statistical study of the environment around Polar Ring Galaxies is presented. Two kinds of search are performed: 1) a study of the concentration and diameters of all the objects surrounding the Polar Rings, within a search field 5 times…

天体物理学 · 物理学 2007-05-23 Chiara Brocca , Daniela Bettoni , Giuseppe Galletta

Polar-ring galaxies (PRGs) are an outstanding example of galaxies with misaligned kinematics where a typically red central galaxy is surrounded by a large-scale ring or disk of stars, gas and dust oriented almost perpendicular to the main…

星系天体物理 · 物理学 2023-10-31 Daniil V. Smirnov , Aleksandr V. Mosenkov , Vladimir P. Reshetnikov

Polar-ring galaxies are photometrically and kinematically decoupled systems which are highly inclined to the major axis of the host galaxy. These objects have been explored since the 1970s, but the rarity of these systems has made such…

I present a catalog of 67 barred galaxies which contain distinct, elliptical stellar structures inside their bars. Fifty of these are double-barred galaxies: a small-scale, "inner" or "secondary" bar is embedded within a large-scale,…

天体物理学 · 物理学 2009-11-10 Peter Erwin

A common point of view is that stable polar structures are mainly present in the E/S0 early-type galaxies lacking dense gas in their host disks. However, nuclear, as well as external polar rings and disks also exist in the late-type hosts,…

星系天体物理 · 物理学 2014-06-19 Alexei Moiseev

Polar ring galaxies are systems with nearly orthogonally rotated components. We have found the gas on polar (or strongly inclined) orbits in two BCD galaxies using ionized gas velocity fields taken with a Fabry-Perot interferometer of the…

宇宙学与河外天体物理 · 物理学 2015-05-19 Alexei Moiseev

Polar-ring galaxies are multi-spin systems, showing star formation in a blue late-type component, perpendicular to a red early-type one, revealing how galaxy formation can sometimes occur in successive steps. We perform two-dimensional…

星系天体物理 · 物理学 2015-06-23 V. Reshetnikov , F. Combes

Aims: We present a statistical analysis of different characteristics of ringed spiral galaxies with the aim of assessing the effects of rings on disk galaxy properties. Methods: We built a catalog of ringed galaxies from the Sloan Digital…

星系天体物理 · 物理学 2021-09-15 Julia Fernandez , Sol Alonso , Valeria Mesa , Fernanda Duplancic , Georgina Coldwell

We have searched for CO lines in a sample of 21 new morphologically determined polar-ring galaxies (of which nine are kinematically confirmed), obtained from a wide search in the Galaxy Zoo project by Moiseev and collaborators. Polar-ring…

宇宙学与河外天体物理 · 物理学 2015-06-15 Francoise Combes , Alexei Moiseev , Vladimir Reshetnikov

The polar ring galaxies (PRGs) represent an interesting type of peculiar systems in which the outer matter is rotating in the plane which is roughly perpendicular to the disk of the main galaxy. Despite the long lasting study of the PRGs…

星系天体物理 · 物理学 2018-03-14 A. Moiseev , S. Khoperskov , A. Khoperskov , K. Smirnova , A. Smirnova , A. Saburova , V. Reshetnikov

Polar-ring galaxies are systems with two nearly orthogonal rotational axes, and are therefore clearly the result of galaxy-galaxy interactions. The host galaxies of polar rings are typically gas-poor early-type systems. The rings…

天体物理学 · 物理学 2007-05-23 Paul B. Eskridge , Richard W. Pogge

Several recent studies indicate that bulges are more complex than merely structureless relaxed stellar systems. We study the HST images of a sample of 130 nearby early type (S0-Sab) disc galaxies and detect pure structureless bulges with…

天体物理学 · 物理学 2008-10-16 Leonel Gutierrez , Antti Tamm , John Beckman , Louis Abramson , Peter Erwin , Melanie Guittet

Polar-ring galaxies (PRGs) are fascinating systems in which the central object (typically, an early-type galaxy) is encircled by a large-scale ring of stars, gas, and dust with almost perpendicular spin. PRGs are rare objects and their…

星系天体物理 · 物理学 2018-12-19 V. P. Reshetnikov , A. V. Mosenkov

General structural properties and low surface brightness tidal features hold important clues to the formation of galaxies. In this paper, we study a sample of polar-ring galaxies (PRGs) based on optical imaging from the Sloan Digital Sky…

星系天体物理 · 物理学 2022-08-30 Aleksandr V. Mosenkov , Vladimir P. Reshetnikov , Maria N. Skryabina , Zacory Shakespear

We present an analysis of structural features of all known galaxies with optical polar rings. We find a clear dichotomy for objects of this peculiar class. Bulge-dominated S0 galaxies possess only short narrow rings, while disk-dominated…

天体物理学 · 物理学 2009-09-25 V. Reshetnikov , N. Sotnikova

Polar ring galaxies (PRGs) host an outer ring of gas and stars oriented nearly perpendicular to the main stellar body. They represent extreme examples of misaligned systems and provide valuable insight into galaxy interactions, gas…

We numerically investigate stellar and gas dynamics in star-forming and dissipative galaxy mergers between two disk galaxies with specific orbital configurations. We find that violent relaxation combined with gaseous dissipation in galaxy…

天体物理学 · 物理学 2009-10-30 Kenji Bekki

We present data for a sample of 45 spiral galaxies over a range of Hubble types, imaged in the near-IR J and K bands. Parameters are calculated describing the bulge, disk and bar K-band light distributions, and we look for correlations…

天体物理学 · 物理学 2007-05-23 M. S. Seigar , P. A. James
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