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Related papers: The Ring Produced by an Extra-Galactic Superbubble…

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We report the discovery of an unusual z=1.14 object, dubbed the $\infty$ galaxy, in JWST imaging of the COSMOS field. Its rest-frame near-IR light is dominated by two compact nuclei with stellar masses of $\sim 10^{11}$ Msun and a projected…

The Sun is located inside an extremely low density region of quite irregular shape called the Local Bubble. Close to the Local Bubble, there is an even larger cavity known as Loop I. A ring-like feature observed in X-ray and HI has been…

Astrophysics · Physics 2009-11-13 W. Reis , W. J. B. Corradi

We report the discovery of a partial Einstein ring of radius 1.48arcsec produced by a massive (and seemingly isolated) elliptical galaxy. The spectroscopic follow-up at the VLT reveals a 2L* galaxy at z=0.986, which is lensing a…

Astrophysics · Physics 2007-05-23 R. A. Cabanac , D. Valls-Gabaud , A. O. Jaunsen , C. Lidman , H. Jerjen

We present images of the peculiar galaxy Arp~10 which reveal two rings of concurrent star formation. Apart from a bright ring visible on early photographs of the system, an even brighter inner ring of \ion{H}{2} regions is found within the…

Astrophysics · Physics 2014-10-13 V. Charmandaris , P. N. Appleton , A. P. Marston

(abridged) An object classified as a galaxy in on-line data bases and revealed on sky survey images as a distant ring galaxy is a rare case of polar ring galaxy where the ring is only slightly inclined to the equatorial plane of the central…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 Noah Brosch , Alexei Y. Kniazev , Alexei Moiseev , Simon A. Pustilnik

Backward terahertz radiation can be produced by a high-intensity laser normally incident upon an underdense plasma. It is found that terahertz radiation is generated by electrons refluxing along the bubble shell. These shell electrons have…

Plasma Physics · Physics 2019-05-01 J. F. Qu , X. F. Li , X. Y. Liu , P. Liu , Y , J. Song , Z. Fu , Q. Yu , Q. Kong

A family of potential-density pairs that represent spherical shells with finite thickness is obtained from the superposition of spheres with finite radii. Other families of shells with infinite thickness with a central hole are obtained by…

General Relativity and Quantum Cosmology · Physics 2010-11-01 D. Vogt , P. S. Letelier

We present UBR and H$\alpha$ imaging of NGC 1620, a highly inclined spiral galaxy that contains a large scale, arc-like feature of radius 3 kpc in its outer disk at a distance of $\sim$ 11 kpc from the center. What is unusual about this…

Astrophysics · Physics 2009-10-22 J. Patricia Vader , Brian Chaboyer

Galactic outflows from local starburst galaxies typically exhibit a layered geometry, with cool $10^4\,$K flow sheathing a hotter $10^7\,$K, cylindrically-collimated, X-ray emitting plasma. Here, we argue that winds driven by…

Astrophysics of Galaxies · Physics 2022-08-22 Dustin D. Nguyen , Todd A. Thompson

We report the discovery of an almost complete Einstein ring of diameter 10" in Sloan Digital Sky Survey (SDSS) Data Release 5 (DR5). Spectroscopic data from the 6m telescope of the Special Astrophysical Observatory reveals that the…

The galactic supershells are cavities in the interstellar medium. These shells can be explained by introducing the concept of superbubbles, the theoretical result of multiple supernova. The superbubbles can be analytically described if the…

Astrophysics · Physics 2015-06-24 Lorenzo Zaninetti

We develop a dynamical theory for the origin of nuclear rings in barred galaxies. In analogy with the standard theory of accretion discs, our theory is based on shear viscous forces among nested annuli of gas. However, the fact that gas…

We hypothesise that dust rings in protoplanetary discs formed by an embedded planet should have properties that reflect the planet's mass. We use 2D hydrodynamical simulations of planet-disc interactions to investigate this, focusing on…

Earth and Planetary Astrophysics · Physics 2026-05-28 Amena Faruqi , Jessica Speedie , Ralph E. Pudritz , Farzana Meru

On the basis of ``sticky particle'' calculations, it is argued that the gas features observed within 10 pc of the Galactic Centre-- the circumnuclear disk (CND) and the ionized gas filaments-- as well as the newly formed stars in the inner…

Astrophysics · Physics 2009-10-30 R. H. Sanders

Gravitational instabilities play an important role in structure formation of gas-rich high-redshift disc galaxies. In this paper, we revisit the axisymmetric perturbation theory and the resulting growth of structure by taking the realistic…

Astrophysics of Galaxies · Physics 2015-02-04 Manuel Behrendt , Andreas Burkert , Marc Schartmann

Taking into account that the real quantum materials are engineered generically at a finite chemical potential, we investigate the Einstein ring structure for the lensed response of the complex scalar field as a probe wave on the charged AdS…

High Energy Physics - Theory · Physics 2022-11-23 Yuxuan Liu , Qian Chen , Xiao-Xiong Zeng , HongBao Zhang , Wen-Liang Zhang

The construction of complex rotation numbers, due to V.Arnold, gives rise to a fractal-like set "bubbles" related to a circle diffeomorphism. "Bubbles" is a complex analogue to Arnold tongues. This article contains a survey of the known…

Dynamical Systems · Mathematics 2018-06-06 Nataliya Goncharuk

Using three-dimensional particle-in-cell simulations we show that a strongly nonlinear plasma wave excited by an ultrahigh intensity laser pulse works as a compact high-brightness source of X-ray radiation. It has been recently suggested by…

Optics · Physics 2007-05-23 S. Kiselev , A. Pukhov , I. Kostyukov

Star formation is enhanced in spiral arms because of a combination of orbit crowding, cloud collisions, and gravitational instabilities. The characteristic mass for the instability is 10^7 Msun in gas and 10^5 Msun in stars, and the…

Astrophysics · Physics 2015-05-13 Bruce G. Elmegreen

Using Chandra and HST we show that X-ray and H$\alpha$ filaments that form the 1.3-kpc diameter superbubble of NGC 3079 have strikingly similar patterns at 0."8 resolution. This tight match seems to arise from cool disk gas that has been…

Astrophysics · Physics 2009-11-07 G. Cecil , J. Bland-Hawthorn , S. Veilleux