Zobrazeno 1 - 10
of 14
pro vyhledávání: '"Sander Valcke"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 408:71-86
In this paper we investigate whether Smoothed Particle Hydrodynamics (SPH), equipped with artificial conductivity, is able to capture the physics of density/energy discontinuities in the case of the so-called shearing layers test, a test for examinin
Publikováno v:
Astronomische Nachrichten. 330:972-977
We present models of the formation and evolution of isolated dwarf galaxies. The models follow the evolution of an initially homogeneous gas cloud collapsing in a pre-existing dark-matter halo. These simplified initial conditions are supported by the
Publikováno v:
Proceedings of the International Astronomical Union. 4:318-322
We investigate the global photometric scaling relations traced by early-type galaxies in different environments, ranging from dwarf spheroidals, over dwarf elliptical galaxies, up to giant ellipticals (−8 mag ≳ MV ≳ −24 mag). These results ar
Publikováno v:
EAS Publications Series. 48:407-409
dIrrs and flat, rotating dEs generally possess flat metallicity profiles while round dEs show strong metallicity gradients [8]. Unlike dEs, dIrrs also exhibit ongoing star formation (SF) [4], compatible with a continuous star formation history (SFH).
ERRATUM: 'EFFICIENT THREE-DIMENSIONAL NLTE DUST RADIATIVE TRANSFER WITH SKIRT' (2011, ApJS, 196, 22)
Autor:
Edgardo Vidal Pérez, Maarten Baes, Waad Saftly, Ilse De Looze, Marko Stalevski, Sander Valcke, Jacopo Fritz, Joris Verstappen
Publikováno v:
The Astrophysical Journal Supplement Series. 223:17
Publikováno v:
Monthly Notices of the Royal Astronomical Society.
We show results based on a large suite of N-Body/SPH simulations of isolated, flat dwarf galaxies, both rotating and non-rotating. The main goal is to investigate possible mechanisms to explain the observed dichotomy in radial stellar metallicity pro
Publikováno v:
AIP Conference Proceedings.
We have constructed a series of models to investigate the influence of tidal forces on the formation and evolution of dwarf spheroidal galaxies. These Nbody/SPH models consist of a model for an isolated dwarf spheroidal galaxy which is placed on an o
Publikováno v:
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
We present new fully self-consistent models of the formation and evolution of isolated dwarf galaxies. We have used the publicly available N-body/SPH code HYDRA, to which we have added a set of star formation criteria, and prescriptions for chemical
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::982194f407bc85801bd13bc7d3c0a443
http://arxiv.org/abs/0807.0397
http://arxiv.org/abs/0807.0397
We investigate the global photometric scaling relations traced by early-type galaxies in different environments, ranging from dwarf spheroidals, over dwarf elliptical galaxies, up to giant ellipticals (-8 mag > M_V > -24 mag). These results are based
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fa3cb671a23de474846bd247491e41f9
Publikováno v:
EAS Publications Series. 48:405-406
We have investigated whether Smoothed Particle Hydrodynamics (SPH), equipped with artificial conductivity, is able to capture the physics of density/energy discontinuities in the case of the so-called shearing layers test, a test for examining Kelvin