scholarly journals Collisional Ring Galaxies in Small Groups

2000 ◽  
Vol 174 ◽  
pp. 277-280
Author(s):  
C. Horellou

AbstractThe probability of plunging orbits is enhanced in groups of galaxies and indeed, observations show that ring galaxies, which are believed to form when a galaxy passes through the center of a larger rotating disk, are often found in small groups. Numerical simulations combined with a knowledge of the large-scale H I distribution provide strong constraints on the dynamical history of these systems and on the identity of the intruder. Here we present a numerical model of the Cartwheel galaxy which supports the suggestion that the most distant companion is the intruder. We also present high-resolution H I observations of the more irregular system Arp 119 that reveal a possible connection to the most distant companion.

Author(s):  
Arthur Holland Michel

As we find ourselves bearing witness—even in our own backyards—to what is increasingly being referred to as the “drone revolution,” it might be a good time to turn our attention back in time and figure out how, exactly, we got here. The large-scale use of drones for national defense and law enforcement is a relatively recent development, but unmanned aerial surveillance draws from a doctrine that is as old as flight itself. Though the fundamental logic of aerial surveillance has remained the same—to put an eye in the sky so that one may look down upon one’s enemies—the technology has evolved dramatically over this period, driving shifts in aerial surveillance theory and practice. New technologies enable new techniques that, in turn, inspire new ways of thinking about how to spy from the sky, and produce new experiences for those being watched. Our present drone revolution, which has itself driven what is being called the “intelligence, surveillance, and reconnaissance (ISR) revolution,” is the result of this process played out over an entire century. The unmanned aerial spying efforts of the United States military and intelligence community have a particularly long and influential history, beginning with the Union Army’s manned observation balloon corps of the Civil War. Our story begins, in earnest, with fragile and failure-prone “aerial torpedos” in the First World War and an innovative and overlooked live video transmission system from the 1930s, through the CIA’s little-known—and radically forward-thinking—Samos spy satellite program of the late 1950s and a series of extraordinarily ambitious Cold War drone programs, up to the adoption of drones over Bosnia in the 1990s. Together, these episodes show how we got the drones of today and realized the core principles that define aerial spycraft (that is, how to find and watch “the bad guys”) in the 21st century: cover as much ground as possible; process and disseminate what you collect as quickly as possible, ideally, as close as you can get to real-time; and be as persistent as possible. The drones and high-resolution aerial cameras that are finding their way into the tool-kits of police departments will bring these principles along with them. Even if the growing number of law enforcement officers now using this technology aren’t fully aware of the long legacy of aerial surveillance that they are joining, the influence of this formative history of surveillance on their aerial crime-fighting operations is evident. Just as aerial surveillance transformed the battlefield, it will have a similarly profound effect on the experience and tactics of those operating the cameras, as well as, crucially, those individuals being watched by them. By grasping this history, we can better understand not only why and how drones are being used to fight crime, but also what to expect when every police department in the country owns an eye in the sky.


2015 ◽  
Vol 8 (6) ◽  
pp. 1831-1838 ◽  
Author(s):  
N. M. Gavrilov ◽  
S. P. Kshevetskii ◽  
A. V. Koval

Abstract. Comparisons of amplitudes of wave variations of atmospheric characteristics obtained using direct numerical simulation models with polarization relations given by conventional theories of linear acoustic-gravity waves (AGWs) could be helpful for testing these numerical models. In this study, we performed high-resolution numerical simulations of nonlinear AGW propagation at altitudes 0–500 km from a plane wave forcing at the Earth's surface and compared them with analytical polarization relations of linear AGW theory. After some transition time te (increasing with altitude) subsequent to triggering the wave source, the initial wave pulse disappears and the main spectral components of the wave source dominate. The numbers of numerically simulated and analytical pairs of AGW parameters, which are equal with confidence of 95 %, are largest at altitudes 30–60 km at t > te. At low and high altitudes and at t < te, numbers of equal pairs are smaller, because of the influence of the lower boundary conditions, strong dissipation and AGW transience making substantial inclinations from conditions, assumed in conventional theories of linear nondissipative stationary AGWs in the free atmosphere. Reasonable agreements between simulated and analytical wave parameters satisfying the scope of the limitations of the AGW theory prove the adequacy of the used wave numerical model. Significant differences between numerical and analytical AGW parameters reveal circumstances when analytical theories give substantial errors and numerical simulations of wave fields are required. In addition, direct numerical AGW simulations may be useful tools for testing simplified parameterizations of wave effects in the atmosphere.


2018 ◽  
Vol 40 ◽  
pp. 05042
Author(s):  
Go Morikawa ◽  
Ichiro Kimura

The objective of this study is to verify the validity of a hyper grid type (double grid model) computational model, for calculating flood flows with inundations. Nowadays, detailed information of the bathymetry is available due to improved measurement techniques, such as LP data. However, the number of grid cells used in the computation is limited because of the limitation of computational infrastructures. A double grid approach based on the model proposed by Volp et. al.(2013) is employed to overcome this problem.This model directly uses the high resolution topographic data though the discretization of the governing equations are made on coarser grid. The computational results showed that the present numerical model can compute the large scale flood phenomena efficiently and accurately.


2021 ◽  
Author(s):  
YuanJung Tsai ◽  
WeiLin Lee

&lt;p&gt;In 2009, a large-scale landslide was triggered by typhoon rainfall and buried an entire village, which named Hsiaolin and located in Taiwan.&amp;#160;&lt;br&gt;After that, Soil and Water Conservation Bureau (SWCB) has promoted a national project for the prevention work of large-scale landslide. The national project includes with the investigation of potential area, the design of monitoring system, and the design of warning system, etc.&amp;#160;&lt;br&gt;The investigation of potential large-sclae landslide was based on the &amp;#160;digital elevation model with 1 meter resolution. However, the investigation of the underground was lack and not clear enough. Therefore, the specific landslide's body is hardly to estimate and it causes difficulty in follow-up works.&amp;#160;&lt;br&gt;This study applied two methods to investigate the scenario of slope failure. The first method is based on the limited equilibrium method, which proposed by Yoshino and Uchida (2019). The method was used to search the specific region of unstable slope based on a series of high-resolution digital elevation models. After the specific region of unstable slope was confirmed, the landslide can be simulated by a numerical model, which this study proposed to represent the entire landslide process from occurrence to post-failure .&amp;#160;&lt;br&gt;These proposed methods were applied at Baolai area, south Taiwan to track the evolution of the potential area. The failure scenario could be evaluated by the proposed numerical model. By this study, the investigation of underground can be evaluated and these results are very important information for the design of monitoring system.&lt;/p&gt;


2022 ◽  
Author(s):  
Elise Parey ◽  
Alexandra Louis ◽  
Jerome Monfort ◽  
Yann Guiguen ◽  
Hugues Roest Crollius ◽  
...  

Teleost fish are one of the most species-rich and diverse clades amongst vertebrates, which makes them an outstanding model group for evolutionary, ecological and functional genomics. Yet, despite a growing number of sequence reference genomes, large-scale comparative analysis remains challenging in teleosts due to the specifics of their genomic organization. As legacy of a whole genome duplication dated 320 million years ago, a large fraction of teleost genomes remain in duplicate paralogous copies. This ancestral polyploidy confounds the detailed identification of orthologous genomic regions across teleost species. Here, we combine tailored gene phylogeny methodology together with the state-of-the art ancestral karyotype reconstruction to establish the first high resolution comparative atlas of paleopolyploid regions across 74 teleost fish genomes. We show that this atlas represents a unique, robust and reliable resource for fish genomics. We then use the comparative atlas to study the tetraploidization and rediploidization mechanisms that affected the ancestor of teleosts. Although the polyploid history of teleost genomes appears complex, we uncover that meiotic recombination persisted between duplicated chromosomes for over 60 million years after polyploidization, suggesting that the teleost ancestor was an autotetraploid.


1988 ◽  
Vol 130 ◽  
pp. 409-420
Author(s):  
Marc Aaronson ◽  
Edward W. Olszewski

We begin by reviewing the history of Aaronson's entry into the study of dark matter and velocity dispersions. A short review of mass estimations and dark matter in spirals, small groups of galaxies, dwarf irregulars, and dwarf spirals follows. We then discuss velocity dispersions in the five dwarf spheroidals Fornax, Carina, Sculptor, Draco, and Ursa Minor. A new velocity histogram for Draco and Ursa Minor is shown. We then end with some questions and theoretical and observational needs.


1988 ◽  
Vol 101 ◽  
pp. 403-406
Author(s):  
M.L. McColloug ◽  
S.L. Mufson

AbstractHigh resolution observations at radio, infrared, optical and X-ray wavelengths have been made (Mufson et al. 1986). The infrared spectrum determined from the IRAS observations has been fitted with models which include shock heated dust, infrared line emission, and radiatively heated dust emission. Numerical simulations of a supernova expanding into a uniform medium, which describe the X-ray and large scale radio emission, are presented.


2019 ◽  
Vol 627 ◽  
pp. A136 ◽  
Author(s):  
E. Iodice ◽  
M. Sarzi ◽  
A. Bittner ◽  
L. Coccato ◽  
L. Costantin ◽  
...  

The 31 brightest galaxies (mB ≤ 15 mag) inside the virial radius of the Fornax cluster were observed from the centres to the outskirts with the Multi Unit Spectroscopic Explorer on the Very Large Telescope. These observations provide detailed high-resolution maps of the line-of-sight kinematics, line strengths of the stars, ionised gas reaching 2–3 Re for 21 early-type galaxies, and 1–2 Re for 10 late-type galaxies. The majority of the galaxies are regular rotators, with eight hosting a kinematically distinct core. Only two galaxies are slow rotators. The mean age, total metallicity, and [Mg/Fe] abundance ratio in the bright central region inside 0.5 Re and in the galaxy outskirts are presented. Extended emission-line gas is detected in 13 galaxies, most of them are late-type objects with wide-spread star formation. The measured structural properties are analysed in relation to the galaxies’ position in the projected phase space of the cluster. This shows that the Fornax cluster appears to consist of three main groups of galaxies inside the virial radius: the old core; a clump of galaxies, which is aligned with the local large-scale structure and was accreted soon after the formation of the core; and a group of galaxies that fell in more recently.


Sign in / Sign up

Export Citation Format

Share Document