Tides and Arp's hypothesis about distribution of Hii regions

We discuss Arp's hypothesis that the HII regions are more numerous and more conspicuous on the side of a galaxy facing its companion. Arp's hypothesis seems not to be true if we add to Hodge's sets of galaxies only the most probably tidally-interacting cases.     

The asymmetry of the velocity distribution in the rotating ring in U Gem stars

It is shown that the non-keplerian character of the rotation of the ring of gas particles in a close binary system gives too large an amplitude of the radial velocity curve if this amplitude is determined from the positions of the emission lines of the ring.     

Precipitation,temperature and wind in Norway: dynamical downscaling of ERA40

A novel downscaling approach of the ERA40 (ECMWF 40-years reanalysis) data set has been taken and results for comparison with observations in Norway are shown. The method applies a nudging technique in a stretched global model, focused in the Norwegian Sea (67°N, 5°W). The effective resolution is three times the one of the ERA40, equivalent to about 30 km grid spacing in the area of focus. Longer waves (<T42) in the downscaled solution are nudged towards the ERA40 solution, and thus the large-scale circulation is similar in the two data sets. The shorter waves are free to evolve, and produce high intensities of winds and precipitation. The comparison to observations incorporate numerous station data points of (1) precipitation (#357), (2) temperature (#98) and (3) wind (#10), and for the period 1961–1990, the downscaled data set shows large improvements over ERA40. The daily precipitation shows considerable reduction in bias (from 50 to 11%), and twofold reduction at the 99.9 percentile (from −59 to −29%). The daily temperature showed a bias reduction of about a degree in most areas, and relative large RMSE reduction (from 7.5 to 5.0°C except winter). The wind comparison showed a slight improvement in bias, and significant improvements in RMSE.     

CO 2 emission trading model with trading prices

In this paper we consider the buying/selling prices of carbon dioxide (CO₂) emission permits in trading models with uncertainty. Permission prices, although usually omitted from standard models, may significantly influence the trading market. We thus undertook to construct a more realistic trade model and to compare it with the standard one. To do this, we introduced several important changes to the standard model, namely, (1) a new optimized quality function; and (2) transactions with price negotiations between regions. We also enhanced the model using methods described in the literature to allow it to deal with reported emissions uncertainty. Additionally, we used an original method of simulating this kind of market based on a specialized evolutionary algorithm (EA).     

The STAGES view of red spirals and dusty red galaxies: mass-dependent quenching of star formation in cluster infall

We investigate the properties of optically passive spirals and dusty red galaxies in the A901/2 cluster complex at redshift ∼0.17 using rest-frame near-ultraviolet–optical spectral energy distributions, 24-μm infrared data and Hubble Space Telescope morphologies from the STAGES data set. The cluster sample is based on COMBO-17 redshifts with an rms precision of  σ _cz ≈ 2000 km s⁻¹  . We find that 'dusty red galaxies' and 'optically passive spirals' in A901/2 are largely the same phenomenon, and that they form stars at a substantial rate, which is only four times lower than that in blue spirals at fixed mass. This star formation is more obscured than in blue galaxies and its optical signatures are weak. They appear predominantly in the stellar mass range of  log  M _*/M_⊙=[10, 11]  where they constitute over half of the star-forming galaxies in the cluster; they are thus a vital ingredient for understanding the overall picture of star formation quenching in clusters. We find that the mean specific star formation rate (SFR) of star-forming galaxies in the cluster is clearly lower than in the field, in contrast to the specific SFR properties of blue galaxies alone, which appear similar in cluster and field. Such a rich red spiral population is best explained if quenching is a slow process and morphological transformation is delayed even more. At  log  M _*/M_⊙ < 10  , such galaxies are rare, suggesting that their quenching is fast and accompanied by morphological change. We note that edge-on spirals play a minor role; despite being dust reddened they form only a small fraction of spirals independent of environment.     

Application of electron paramagnetic resonance spectroscopy to examination of carbonized coal blends

Paramagnetic centers in two- and three-component coal blends carbonized at 1000 °C were studied by X-band (9.3 GHz) electron paramagnetic resonance (EPR) technique. The blends were prepared from three different Polish coals with carbon contents [wt.%]: 88.66, 86.21, and 82.67, respectively. The aim of this work was to compare EPR parameters and concentrations of paramagnetic centers in the initial and carbonized coal samples. Furthermore the spin–spin and spin–lattice interactions were characterized.EPR spectra were measured with magnetic modulation 100 kHz and microwave power 0.7 mW. Amplitudes and linewidths of EPR spectra were obtained. g-Factors were calculated from resonance condition. Concentrations of paramagnetic centers in the samples were determined. Influence of microwave power in the range 0.7–70 mW on EPR spectra was analyzed.All the studied samples revealed paramagnetism. Unpaired electrons are localized in the same atoms, because similar g-values in the range 2.0035–2.0038 were obtained for all the original samples. The EPR parameters of coal blends were additive in comparison with the parent coals. EPR spectra strongly changed after carbonization of the coal samples. Narrower EPR lines were measured for the original coal samples than for carbonized ones. We detected lower concentrations of paramagnetic centers in carbonized three-component coal blends than in two-component carbonized blends. EPR lines of the studied carbonized blends were not saturated at the microwave power used, which suggests fast spin–lattice relaxation processes in the samples. EPR examination proved chemical interactions between coal constituents during carbonization of coal blends.     

The dark matter environment of the Abell 901/902 supercluster: a weak lensing analysis of the HST STAGES survey

We present a high-resolution dark matter reconstruction of the   z = 0.165  Abell 901/902 supercluster from a weak lensing analysis of the Hubble Space Telescope STAGES survey. We detect the four main structures of the supercluster at high significance, resolving substructure within and between the clusters. We find that the distribution of dark matter is well traced by the cluster galaxies, with the brightest cluster galaxies marking out the strongest peaks in the dark matter distribution. We also find a significant extension of the dark matter distribution of Abell 901a in the direction of an infalling X-ray group Abell 901α. We present mass, mass-to-light and mass-to-stellar mass ratio measurements of the structures and substructures that we detect. We find no evidence for variation of the mass-to-light and mass-to-stellar mass ratio between the different clusters. We compare our space-based lensing analysis with an earlier ground-based lensing analysis of the supercluster to demonstrate the importance of space-based imaging for future weak lensing dark matter 'observations'.     

Landslide features identification and morphology investigation using high-resolution DEM derivatives

Natural Hazards - In the last decade, development in remote sensing techniques has opened new avenues for studying the evolution of landscapes dominated by mass wasting processes. Conventional...     

Das Neokom in Polen und seine paläogeographische Bedeutung

Zusammenfassung Die geologische Geschichte Nordwest-Polens zur Zeit der unteren Kreide kann in allgemeinen Zügen folgenderma\en dargestellt werden:Gegen Ende des Jura, ungefähr zur Zeit des Münder Mergels, sind hier Bewegungen eingetreten, die das Land teilweise trockengelegt und der Denudation preisgegeben haben. In den durch die Bewegungen gebildeten Senken blieben Lagunen erhalten, deren einige brackisches Wasser führten, während in anderen durch Eindampfung Gipslager abgesetzt wurden. Der Serpulit brachte eine positive Meeresbewegung mit, die sich im Infravalanginian derart verstärkte, da\ sich seine Ablagerungen nicht nur in den alten Senken kontinuierlich auf dem Serpulit abgesetzt, sondern auch auf denudierte, früher gehobene Schollen transgressiv ausgebreitet haben. Die Infravalanginian-See war brackisch und hat in NW-Polen typische Wealdenablagerungen abgesetzt, bei Tomaszów aber, etwas südlicher, ist das Infravalangian zwar litoral, aber rein marin ausgebildet, wobei es viele ähnlichkeit mit dem Infravalangian der Teschener Karpathen aufweist. Die Wealdensee und das karpathische Meer waren durch einen Sund verbunden, der sich über Tomaszów längs dem Polnischen Mittelgebirge gegen die Karpathen hinzog. Im Valanginian erreicht die neokome Transgression ihren Höhepunkt, es werden dunkle Tone mit reicher Hilsfauna abgesetzt; wahrscheinlich hat sich diese Transgression von Ru\land über die Polesje-Schwelle und über das westliche Polen nach Deutschland und weiter bis nach Ost-England erstreckt. Das polnische Becken stand in direkter Verbindung mit dem nordwestdeutschen; es war ebenfalls, obwohl dürftiger, mit dem karpathischen Meere verbunden; gerade hier ist der Weg zu suchen, den die Migrationen der nördlichen Elemente ins alpine Becken eingeschlagen haben. Im oberen Valanginian fängt eine Regression an, die in Zentral-Ru\land einsetzt und zu dessen Trockenlegung und zum Abschlu\ der Verbindung des polnischen Beckens mit dem Osten führt. Mit dem Anfang des Hauterivians macht sich die Regression auch in Polen fühlbar und verursacht die Verflachung des Meeres in Polen sowie den Abbruch der Verbindung mit dem karpathischen Meere, in welchem von nun ab keine nordischen eingewanderten Faunenelemente mehr erscheinen. Im oberen Hauterivian zieht sich das Meer von Polen und NO-Deutschland zurück. Auf dem neuen Lande herrscht mächtige Denudation, deren gröbere Produkte sich als sehr mächtige Flu\- und Seesande anhäufen. Das Landstadium dauert während des ganzen BarrÊme, Apt und eines Teiles des Albians an, bis zum Anfang der gro\en Gault-Transgression, die wieder in die Senken vordringt.