Results 61 to 70 of about 7,209 (178)
Spin alignments of spiral galaxies within the large-scale structure from SDSS DR7
, 2014 Using a sample of spiral galaxies selected from the Sloan Digital Sky Survey Data Release 7 (SDSS DR7) and Galaxy Zoo 2 (GZ2), we investigate the alignment of spin axes of spiral galaxies with their surrounding large scale structure, which is ...
Bosch, Frank C. van den +6 more
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Fenomenologia de arquitetura. Discursos de Christian Norberg-Schulz e Juhani Pallasmaa
RevistArquis, 2019 Na teoria arquitetónica, a fenomenologia entende-se como um movimento que investiga a arquitetura enquanto experiência humana. Dentro desse movimento, este artigo destaca dois discursos: o de Christian Norberg-Schulz e de Juhani Pallasmaa por ...
Ricardo Chaves Hernández
doaj +1 more source
Contents and Space: New Concept and New Building of the Militärhistorisches Museum of the Bundeswehr
Museum & Society, 2012 The Bundeswehr Museum of Military History in the north of Dresden will be the largest military history museum in Germany. Before German reunification, the museum buildings housed the Museum of the National People’s Army. Its collections and premises were
Gorch Pieken
doaj
The Problem of Temporality in the Architectural Heritage
Дискурс, 2020 Introduction. As a spatial art, architecture is related to the past, the present and, thanks to its monumentality, is fixed in the foreseeable future.
A. V. Yurieva
doaj +1 more source
, 2014 Observations have shown that the spatial distribution of satellite galaxies is not random, but aligned with the major axes of central galaxies. This alignment is dependent on galaxy properties, such that red satellites are more strongly aligned than blue
Dutton, Aaron +5 more
core +1 more source
Tensor anisotropy as a tracer of cosmic voids
, 2015 We present a new method to find voids in cosmological simulations based on the tidal and the velocity shear tensors definitions of the cosmic web. We use the fractional anisotropy (FA) computed from the eigenvalues of each web scheme as a void tracer. We
Bustamante, Sebastian +1 more
core +1 more source
Why do galactic spins flip in the cosmic web? A Theory of Tidal Torques near saddles
, 2014 Filaments of the cosmic web drive spin acquisition of disc galaxies. The point process of filament-type saddle represent best this environment and can be used to revisit the Tidal Torque Theory in the context of an anisotropic peak (saddle) background ...
Codis, Sandrine +5 more
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Frente a líneas que no dejan nada atrás
RevistArquis, 2013 Presentación Este texto es un lúcido cuestionamiento de la noción de “interpretación” en la representación arquitectónica, entendida comúnmente como el desvelamiento de un supuesto significado que yace oculto entre los misterios de la obra y el turbio ...
Robin Evans
doaj
Line-of-Sight Mass Estimator and the Masses of the Milky Way and Andromeda Galaxy
UniverseThe total mass of a galaxy group, such as the Milky Way (MW) and the Andromeda Galaxy (M 31), is typically determined from the kinematics of satellites within their virial zones. Bahcall and Tremaine (1981) proposed the v2r estimator as an alternative to
Danila Makarov +3 more
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Filaments from the galaxy distribution and from the velocity field in the local universe
, 2015 The cosmic web that characterizes the large-scale structure of the Universe can be quantified by a variety of methods. For example, large redshift surveys can be used in combination with point process algorithms to extract long curvilinear filaments in ...
Courtois, Helene +4 more
core +3 more sources