Zobrazeno 1 - 10
of 17
pro vyhledávání: '"Devin W. Silvia"'
Autor:
Devin W. Silvia, Marcos D. Caballero, Thomas Finzell, Rachel Frisbie, Patti Hamerski, Emily Bolger, Sarah Castle, Rachel Roca, Paige Tourangeau
Publikováno v:
Proceedings of the 54th ACM Technical Symposium on Computer Science Education V. 2.
Publikováno v:
Proceedings of the 54th ACM Technical Symposium on Computer Science Education V. 2.
Publikováno v:
Lecture Notes in Computer Science ISBN: 9783030227494
ICCS (5)
ICCS (5)
One of the core missions of Michigan State University’s new Department of Computational Mathematics, Science, and Engineering is to provide education in computational modeling and data science to MSU’s undergraduate and graduate students. In this
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7925e0e41e1a24a3042b5d2be968484a
https://doi.org/10.1007/978-3-030-22750-0_30
https://doi.org/10.1007/978-3-030-22750-0_30
Autor:
Jessica K. Werk, Britton D. Smith, Cameron Hummels, Philip F. Hopkins, John H. Wise, Nicolas Lehner, Iryna S. Butsky, Brian W. O'Shea, David C. Collins, Devin W. Silvia
Publikováno v:
Hummels, C B, Smith, B D, Hopkins, P F, O'Shea, B W, Silvia, D W, Werk, J K, Lehner, N, Wise, J H, Collins, D C & Butsky, I S 2019, ' The Impact of Enhanced Halo Resolution on the Simulated Circumgalactic Medium ', Astrophysical Journal . https://doi.org/10.3847/1538-4357/ab378f
Traditional cosmological hydrodynamics simulations fail to spatially resolve the circumgalatic medium (CGM), the reservoir of tenuous gas surrounding a galaxy and extending to its virial radius. We introduce the technique of Enhanced Halo Resolution
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::590c1b58a12b37e9b6c60eb2a855aba8
http://arxiv.org/abs/1811.12410
http://arxiv.org/abs/1811.12410
Trident: a universal tool for generating synthetic absorption spectra from astrophysical simulations
Hydrodynamical simulations are increasingly able to accurately model physical systems on stellar, galactic, and cosmological scales, however, the utility of these simulations is often limited by our ability to directly compare them with the datasets
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9eec906727837bbadc4353f44721fa94
Aims. Adaptive optics images are used to test the hypothesis that the explosive BN/KL outflow from the Orion OMC1 cloud core was powered by the dynamical decay of a non-hierarchical system of massive stars. Methods. Narrow-band H2, [Fe II], and broad
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bec3e96ac093167f7dce41237e4547ab
http://arxiv.org/abs/1502.04711
http://arxiv.org/abs/1502.04711
Autor:
Britton D. Smith, Devin W. Silvia, Matthew J. Turk, Steinn Sigurdsson, Brian W. O’Shea, J. Michael Shull, Michael L. Norman, Daniel J. Whalen, Volker Bromm, Naoki Yoshida
Publikováno v:
AIP Conference Proceedings.
We study how the collapse of gas clouds is altered by the addition of metals by performing a series of simulations of pre‐enriched star formation at various metallicities using the adaptive mesh refinement code Enzo. In order to directly compare wi
We investigate through hydrodynamic simulations the destruction of newly-formed dust grains by sputtering in the reverse shocks of supernova remnants. Using an idealized setup of a planar shock impacting a dense, spherical clump, we implant a populat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e2602c8c9a1507b8f405ce7ff2a0035c
Autor:
Devin W. Silvia, Eric Agol
The periodic eclipses of the pre-main-sequence binary, KH 15D, have been explained by a circumbinary dust ring inclined to the orbital plane, which causes occultations of the stars as they pass behind the ring edge. We compute the extinction and forw
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b50eafa479552dc81978842e6d204c68
http://arxiv.org/abs/0803.4275
http://arxiv.org/abs/0803.4275
Publikováno v:
The Astrophysical Journal. 736:109
Ejecta knot flickering, ablation tails, and fragmentation are expected signatures associated with the gradual dissolution of high-velocity supernova (SN) ejecta caused by their passage through an inhomogeneous circumstellar or interstellar medium. Su