Zobrazeno 1 - 10
of 23
pro vyhledávání: '"Federico Stasyszyn"'
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
In this work we compare three catalogues of cosmological filaments identified in the Sloan Digital Sky Survey by means of different algorithms by Tempel et al., Pereyra et al., and Mart\'inez et al. We analyse how different identification techniques
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::65194c3c7580830da6c8fd30161d67d7
https://doi.org/10.1093/mnras/staa320
https://doi.org/10.1093/mnras/staa320
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
We study the magnetic fields in galaxy clusters through Faraday rotation measurements crossing systems in different dynamical states. We confirm that magnetic fields are present in those systems and analyze the difference between relaxed and unrelaxe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2ef67826eed1a05ee86918bda4751ebe
https://doi.org/10.1093/mnras/stz1450
https://doi.org/10.1093/mnras/stz1450
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 472:514-531
The formation of massive black hole binaries (MBHBs) is an unavoidable outcome of galaxy evolution via successive mergers. However, the mechanism that drives their orbital evolution from parsec separations down to the gravitational wave (GW) dominate
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ea49e419b24d57bb5fc0d3c54a97e4f3
https://doi.org/10.1093/mnras/stx1996
https://doi.org/10.1093/mnras/stx1996
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
In this work, we identify and analyse the properties of cluster-cluster filaments within a cosmological simulation assuming that they are structures connecting maxima of the density field defined by dark matter halos with masses $M \, \ge 10^{14}\, h
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f0bb343e78e47e62212c77c43df57250
Autor:
Takamitsu Tanaka, Federico Stasyszyn, Pau Amaro-Seoane, F. G. Goicovic, Alberto Sesana, Jorge Cuadra
Publikováno v:
Monthly Notices of the Royal Astronomical Society
There is compelling evidence that most -if not all- galaxies harbour a super-massive black hole (SMBH) at their nucleus, hence binaries of these massive objects are an inevitable product of the hierarchical evolution of structures in the universe, an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3ffe5f05020ab9538d73a8e804174d34
https://doi.org/10.1093/mnras/stv2470
https://doi.org/10.1093/mnras/stv2470
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
We analyse galaxies in groups in the Sloan Digital Sky Survey (SDSS) and find a weak but significant assembly-type bias, where old central galaxies have a higher clustering amplitude (61 $\pm$ 9 per cent) at scales > 1 Mpc than young central galaxies
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::974332f4339a453fb0269dfdc3b29cf5
https://doi.org/10.1093/mnras/stu1318
https://doi.org/10.1093/mnras/stu1318
Autor:
Annette Geng, Hanna Kotarba, Federico Stasyszyn, Klaus Dolag, Alexander M. Beck, Harald Lesch
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 422:2152-2163
An analytical model predicting the growth rates, the absolute growth times and the saturation values of the magnetic field strength within galactic haloes is presented. The analytical results are compared to cosmological MHD simulations of Milky-Way
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b7e5013877576859feb2c9eaf3f29297
https://doi.org/10.1111/j.1365-2966.2012.20759.x
https://doi.org/10.1111/j.1365-2966.2012.20759.x
Autor:
Klaus Dolag, Hanna Kotarba, Annette Geng, Florian Bürzle, Peter Nielaba, Federico Stasyszyn, Alexander M. Beck
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 419:3571-3589
We investigate the magnetic field evolution in a series of galaxy minor mergers using the N-body/smoothed particle hydrodynamics (SPH) code \textsc{Gadget}. The simulations include the effects of radiative cooling, star formation and supernova feedba
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dfc6cefb31739185fb8f3e04e6d2f2af
https://doi.org/10.1111/j.1365-2966.2011.20001.x
https://doi.org/10.1111/j.1365-2966.2011.20001.x
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 418:2234-2250
Magnetic fields in the intra-cluster medium of galaxy clusters have been studied in the past years through different methods. In the next years the up-coming generation of radio telescopes is going to provide new data that have the potential of setti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2ea8223edd1a4007fa793c05c3288511
https://doi.org/10.1111/j.1365-2966.2011.19523.x
https://doi.org/10.1111/j.1365-2966.2011.19523.x
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 417:L61-L65
The protostellar collapse of a molecular cloud core is usually accompanied by outflow phenomena. The latter are thought to be driven by magnetorotational processes from the central parts of the protostellar disc. While several 3D adaptive mesh refine
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3655d07516c00bf182031cd800219672
https://doi.org/10.1111/j.1745-3933.2011.01120.x
https://doi.org/10.1111/j.1745-3933.2011.01120.x