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The formation process, properties, and spatial distribution of galaxy groups and clusters are closely related to the background cosmological model. We use numerical simulations of variants of the CDM model with different cosmological…

Astrophysics · Physics 2007-05-23 Alexander Knebe

In this paper we investigate R-,H-, and M-{\it nw}-selective properties introduced in \cite{BG}. In particular, we provide consistent uncountable examples of such spaces and we define \textit{trivial} R-,H-, and M-{\it nw}-selective spaces…

General Topology · Mathematics 2024-07-29 Maddalena Bonanzinga , Davide Giacopello , Santi Spadaro , Lyubomyr Zdomskyy

In these three lectures a review is provided of the properties of galaxy systems as determined from optical and infrared measurements. Covered topics are: clusters identification, global cluster properties and their scaling relations,…

Astrophysics · Physics 2008-11-24 A. Biviano

It is shown that the unusual thermodynamic properties of matter within the region of two-phase coexistence in hybrid stars result in a change of the standard condition for beginning of convection. In particular, the thermal flux transported…

Solar and Stellar Astrophysics · Physics 2015-12-11 A. V. Yudin , M. Hempel , D. K. Nadyozhin , T. L. Razinkova

In this paper, we give some properties of the Tribonacci and Tribonacci-Lucas quaternions and obtain some identities for them.

Combinatorics · Mathematics 2017-08-18 Ilker Akkus , Gonca Kizilaslan

Various aspects of the connection between cloud cover (CC) and cosmic rays (CR) are analysed. We argue that the anticorrelation between the temporal behaviour of low (LCC) and middle (MCC) clouds evidences against causal connection between…

Earth and Planetary Astrophysics · Physics 2009-06-25 A. D. Erlykin , G. Gyalai , K. Kudela , T. Sloan , A. W. Wolfendale

We characterize certain CR structures of arbitrary codimension (different from 3, 4 and 5) on Riemannian Spin$^c$ manifolds by the existence of a Spin$^c$ structure carrying a strictly partially pure spinor field. Furthermore, we study the…

Differential Geometry · Mathematics 2016-11-11 Rafael Hererra , Roger Nakad

The atmospheric structure of chemically peculiar stars deviates from that of normal stars with similar fundamental parameters due to unusual chemistry, abundance inhomogeneities and the presence of strong magnetic field. These effects are…

Astrophysics · Physics 2007-12-03 O. Kochukhov , D. Shulyak

We discuss phenomenon of simultaneous presence of O- and C-based material in surroundings of evolutionary advanced stars. We concentrate on silicate carbon stars and present observations that directly confirm the binary model scenario for…

Astrophysics · Physics 2007-05-23 R. Szczerba , M. R. Schmidt , M. Pulecka

The photometric properties of the variable stars located in the lower part of the classical instability strip are discussed. The importance of the determination of some light curve parameters and their connection with the stellar models are…

Astrophysics · Physics 2007-05-23 Ennio Poretti , Federica Musazzi

The cellular-Lindel\"of property is a common generalization of the Lindel\"of property and the countable chain condition that was introduced by Bella and Spadaro in 2018. We solve two questions of Alas, Gutierrez-Dominguez and Wilson by…

General Topology · Mathematics 2024-06-21 Rodrigo Hernández-Gutiérrez , Santi Spadaro

We use an action, of 2l-component string links on l-component string links, defined by the first author and Xiao-Song Lin, to lift the indeterminacy of finite type link invariants. The set of links up to this new indeterminacy is in…

Geometric Topology · Mathematics 2010-02-09 Nathan Habegger , Jean-Baptiste Meilhan

The study of the properties of cosmic structures in the universe is one of the most fascinating subject of the modern cosmology research. Far from being predicted, the large scale structure of the matter distribution is a very recent…

Statistical Mechanics · Physics 2016-11-23 L. Pietronero , M. Bottaccio , M. Montuori , F. Sylos Labini

It has become a common practice within the exoplanet field to say that "to know the star is to know the planet." The properties of the host star have a strong, direct influence on the interior and surface conditions of the orbiting planet…

Earth and Planetary Astrophysics · Physics 2024-04-25 Natalie R. Hinkel , Allison Youngblood , Melinda Soares-Furtado

We analyse the strong connections between spaces of vector-valued Lipschitz functions and spaces of linear continuous operators. We apply these links to study duality, Schur properties and norm attainment in the former class of spaces as…

Functional Analysis · Mathematics 2016-07-20 Luis García-Lirola , Colin Petitjean , Abraham Rueda Zoca

In this review article, we argue that our current understanding of the thermodynamic properties of cold QCD matter, originating from first principles calculations at high and low densities, can be used to efficiently constrain the…

Nuclear Theory · Physics 2016-04-20 Eduardo S. Fraga , Aleksi Kurkela , Aleksi Vuorinen

The equation of state provided by effective models of strongly interacting matter should comply with the restrictions imposed by current astrophysical observations on compact stars. Using the equation of state given by the (axial-)vector…

Nuclear Theory · Physics 2021-02-25 János Takátsy , Péter Kovács , György Wolf

Sudden changes in the internal structure of stars, placed at the interface between convective and radiative regions, regions of partial ionisation, or between layers that have acquired different chemical composition as a result of nuclear…

Solar and Stellar Astrophysics · Physics 2021-09-09 Margarida S. Cunha

I discuss some properties of spatially dependent chiral condensates, focusing on one-dimensional modulations. After briefly introducing a generic formalism for studying inhomogeneous solutions in dense quark matter, I consider a plane-wave…

High Energy Physics - Phenomenology · Physics 2018-04-04 Stefano Carignano

We review basic physics of line-driven stellar winds of OB stars. We discuss elementary processes due to which stellar winds are accelerated on a microscopic level. We show how these microscopic processes may enable the outflow and how they…

Astrophysics · Physics 2007-05-23 Jiri Krticka , Jiri Kubat
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