Zobrazeno 1 - 10
of 23
pro vyhledávání: '"Steven Rieder"'
Publikováno v:
Journal of Open Research Software, Vol 1, Iss 1, Pp e9-e9 (2013)
We present MPWide, a light weight communication library which allows efficient message passing over a distributed network. MPWide has been designed to connect application running on distributed (super)computing resources, and to maximize the communic
Externí odkaz:
https://doaj.org/article/a8af9f5309564736893176251a984f48
Publikováno v:
Proceedings of the International Astronomical Union. 16:105-110
We present Ekster, a new method for simulating the formation and dynamics of individual stars in a relatively low-resolution gas background. Here, we use Ekster to simulate star cluster formation in two different regions from each of two galaxy model
Autor:
Alessandro Alberto Trani, Steven Rieder, Ataru Tanikawa, Giuliano Iorio, Riccardo Martini, Georgii Karelin, Hila Glanz, Simon Portegies Zwart
Publikováno v:
Physical Review D, 106(4):043014
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3f16b3b0d1d15f2dc206cead200d6afb
https://hdl.handle.net/1887/3561622
https://hdl.handle.net/1887/3561622
Autor:
Sam Geen, Poojan Agrawal, Paul A. Crowther, B. W. Keller, Alex de Koter, Zsolt Keszthelyi, Freeke van de Voort, Ahmad A. Ali, Frank Backs, Lars Bonne, Vittoria Brugaletta, Annelotte Derkink, Sylvia Ekström, Yvonne A. Fichtner, Luca Grassitelli, Ylva Götberg, Erin R. Higgins, Eva Laplace, Kong You Liow, Marta Lorenzo, Anna F. McLeod, Georges Meynet, Megan Newsome, G. André Oliva, Varsha Ramachandran, Martin P. Rey, Steven Rieder, Emilio Romano-Díaz, Gautham Sabhahit, Andreas A. C. Sander, Rafia Sarwar, Hanno Stinshoff, Mitchel Stoop, Dorottya Szécsi, Maxime Trebitsch, Jorick S. Vink, Ethan Winch
Publikováno v:
Publications of the Astronomical Society of the Pacific, 2023, Vol.135(1044) [Peer Reviewed Journal]
Stars strongly impact their environment, and shape structures on all scales throughout the universe, in a process known as “feedback.” Due to the complexity of both stellar evolution and the physics of larger astrophysical structures, there remai
We present Ekster, a new method for simulating star clusters from birth in a live galaxy simulation that combines the smoothed-particle hydrodynamics (SPH) method Phantom with the $N$-body method PeTar. With Ekster, it becomes possible to simulate in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4547326ebcdfef5912271a650498d13b
http://arxiv.org/abs/2111.09720
http://arxiv.org/abs/2111.09720
Publikováno v:
Proceedings of the International Astronomical Union. 14:216-219
We present a model for hydrodynamic + N-body simulations of star cluster formation and evolution using AMUSE. Our model includes gas dynamics, star formation in regions of dense gas, stellar evolution and a galactic tidal spiral potential, thus incor
Modelling star formation and resolving individual stars in numerical simulations of molecular clouds and galaxies is highly challenging. Simulations on very small scales can be sufficiently well resolved to consistently follow the formation of indivi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1aab5d9293724eaa295c6aa87292064f
Autor:
Alexander J. Bohn, Jozua de Boer, Mark J. Pecaut, Christian Ginski, Steven Rieder, Tiffany Meshkat, Matthew A. Kenworthy, Frans Snik, Eric E. Mamajek, Christoph U. Keller, John Southworth, Maddalena Reggiani
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal Letters, 898(1), L16
Astrophysical Journal Letters, 898(1):L16. IOP Publishing Ltd.
The Astrophysical Journal Letters, 898(1), L16
Astrophysical Journal Letters, 898(1):L16. IOP Publishing Ltd.
Even though tens of directly imaged companions have been discovered in the past decades, the number of directly confirmed multiplanet systems is still small. Dynamical analysis of these systems imposes important constraints on formation mechanisms of
Young massive clusters (YMCs) are the most intense regions of star formation in galaxies. Formulating a model for YMC formation whilst at the same time meeting the constraints from observations is highly challenging however. We show that forming YMCs
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2f396d216d840bc6e43b15da72908ee5
Publikováno v:
Proceedings of the International Astronomical Union. 16:380-381
To form stars in hydrodynamical simulations, we introduce the grouped star formation prescription to convert the grouped sink particles into stars that follow the IMF. We show that this method is robust in different physical scales. Such methods to f