Results 191 to 200 of about 12,706 (233)

Finite-Capacity Thermodynamics of Causal Horizons. [PDF]

Entropy (Basel)
Antiba CA.
europepmc   +1 more source

Gas-phase synthesis of the bicyclic silicon tricarbide molecule (c-SiC₃) as a precursor to silicon carbide nanoparticles in space. [PDF]

Chem Sci
Goettl SJ, Fujioka K, Alves MO, Silva MX, Yang Z, Metya S, Medvedkov IA, Sattasathuchana T, Galvão BRL, Sun R, Kaiser RI.   +10 more
europepmc   +1 more source

<i>Atkinsonella hypoxylon</i> virus capsid structure highlights the diversity of capsid proteins among the <i>Partitiviridae</i>. [PDF]

J Gen Virol
Venturi M, Calthorpe-Byrne M, Aftret B, McNeale D, Rehm BHA, Sainsbury F.   +5 more
europepmc   +1 more source

Gene sequencing and <i>in silico</i> characterization of mannose-binding lectin in South African chicken breeds. [PDF]

J Adv Vet Anim Res
Idowu PA, Mpofu TJ, Zishiri OT, Oluwamayowa OJ, Nephawe KA, Mtileni B.   +5 more
europepmc   +1 more source

Formation time-scales for stellar bars in diverse galactic discs. [PDF]

Mon Not R Astron Soc
Frosst M, Obreschkow D, Ludlow A.
europepmc   +1 more source

Galaxy Tomography with the Gravitational Wave Background from Supermassive Black Hole Binaries

Chen Y.
europepmc   +1 more source

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Galaxies in Interaction

Astronomische Nachrichten, 2004
AbstractPosters: Because of the large number of contributions, some oral presentations had to be transferred into Posters. The reader is referred to the final programme for the actual allocation of Posters.A01 Chemical Enrichment of the Intracluster MediumA02 Structural analysis of high‐velocity clouds – Evidence for an interaction between the Milky ...
Hüttemeister, Susanne, Zeilinger, Werner, Theis, Christian   +2 more
openaire   +1 more source

Galaxy Interactions and the Radio Galaxy Phenomenon

1990
We have been studying powerful radio galaxies (which we define as having radio power at 178MHz, P 178 ≥ 5xl024 Watts/Hz for a cosmology of H o = 100 km sec-1 Mpc-1 and q o = 0) in order to determine their origins. There are two distinct classes of powerful radio galaxies (PRGs), the so called class A and B radio galaxies (Hine and Longair 1979; Heckman
E. P. Smith, T. M. Heckman
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Dynamics of Interacting Galaxies

Annual Review of Astronomy and Astrophysics, 1992
The dynamics of interacting galaxies as observed in the present epoch is reviewed. Topics discussed include numerical methods for modeling galactic interactions, the signatures of interacting galaxies due to tidal forces, and events that add mass to a galaxy.
Joshua E. Barnes, Lars Hernquist
openaire   +2 more sources

Interactions and mergers of galaxies

Resonance, 2007
When two galaxies approach each other, we can witness the effects of the tidal forces on a gigantic scale. Peculiar features like galactic bridges and galactic tails may form, or the two galaxies may even merge into each other and form a single system. Merger of two spiral galaxies leads to the formation of an elliptical galaxy.
S M Alladin, S N Hasan
openaire   +1 more source