Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Punyakoti Ganeshaiah Veena"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 494(3), 3358-3367. Oxford University Press
We determine the mass of the Milky Way bar and the torque it causes, using Gaia DR2, by applying the orbital arc method. Based on this, we have found that the gravitational acceleration is not directed towards the centre of our Galaxy but a few degre
We assess a neural network (NN) method for reconstructing 3D cosmological density and velocity fields (target) from discrete and incomplete galaxy distributions (input). We employ second-order Lagrangian Perturbation Theory to generate a large ensemb
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6349d14e118fad9fa97ebd633fbde988
Autor:
Marius Cautun, Elmo Tempel, Carlos S. Frenk, Rien van de Weygaert, Punyakoti Ganeshaiah Veena
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 503, 2280-2299. Oxford University Press
Monthly notices of the Royal Astronomical Society, 2021, Vol.503(2), pp.2280-2299 [Peer Reviewed Journal]
Monthly Notices of the Royal Astronomical Society, 503(2), 2280-2299
Monthly Notices of the Royal Astronomical Society, 503, 2280-2299. Oxford University Press
Monthly notices of the Royal Astronomical Society, 2021, Vol.503(2), pp.2280-2299 [Peer Reviewed Journal]
Monthly Notices of the Royal Astronomical Society, 503(2), 2280-2299
We explore the evolution of halo spins in the cosmic web using a very large sample of dark matter haloes in the $\Lambda$CDM Planck-Millennium N-body simulation. We use the NEXUS+ multiscale formalism to identify the hierarchy of filaments and sheets
Galaxies can be classified as passive ellipticals or star-forming discs. Ellipticals dominate at the high end of the mass range, and therefore there must be a mechanism responsible for the quenching of star-forming galaxies. This could either be due
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ab28b263fbfb033cafd94fba0613ba25
Autor:
Punyakoti Ganeshaiah Veena
All the celestial objects, from small asteroids and planets to large galaxies and even the long filaments of the cosmic web are rotating. The origin of rotation is yet to be fully understood, especially in the context of galaxies and their dark matte
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::29a866fcdcb4150aa419f6e2fc16a32b
https://research.rug.nl/en/publications/e9eeda77-c5ac-451d-8cb5-c66db0e51707
https://research.rug.nl/en/publications/e9eeda77-c5ac-451d-8cb5-c66db0e51707
Autor:
Punyakoti Ganeshaiah Veena, Rien van de Weygaert, Bernard J. T. Jones, Carlos S. Frenk, Elmo Tempel, Steven Rieder, Marius Cautun
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 481(1), 414-438. Oxford University Press
Monthly notices of the Royal Astronomical Society, 2018, Vol.481(1), pp.414-438 [Peer Reviewed Journal]
Monthly Notices of the Royal Astronomical Society, 481(1), 414-438. Oxford University Press
Monthly notices of the Royal Astronomical Society, 2018, Vol.481(1), pp.414-438 [Peer Reviewed Journal]
We investigate the alignment of haloes with the filaments of the cosmic web using an unprecedently large sample of dark matter haloes taken from the P-Millennium $\Lambda$CDM cosmological N-body simulation. We use the state-of-the-art NEXUS morpholog
Autor:
Marius Cautun, Rien van de Weygaert, Punyakoti Ganeshaiah Veena, Carlos S. Frenk, Elmo Tempel
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 487, 1607-1625. Oxford University Press
Monthly notices of the royal astronomical society, 2019, Vol.487(2), pp.1607-1625 [Peer Reviewed Journal]
Monthly Notices of the Royal Astronomical Society
Monthly notices of the royal astronomical society, 2019, Vol.487(2), pp.1607-1625 [Peer Reviewed Journal]
Monthly Notices of the Royal Astronomical Society
We investigate the alignment of galaxies and haloes relative to cosmic web filaments using the EAGLE hydrodynamical simulation. We identify filaments by applying the NEXUS+ method to the mass distribution and the Bisous formalism to the galaxy distri