Zobrazeno 1 - 10
of 15
pro vyhledávání: '"Tyler Kelley"'
Publikováno v:
Problems and Perspectives in Management, Vol 14, Iss 1, Pp 30-43 (2016)
The paper presents specific examples of leadership training practices and educational activities that have been successfully implemented in an undergraduate program at the U.S. Coast Guard Academy. The purpose of this study is to illustrate a model o
Externí odkaz:
https://doaj.org/article/dba5b7cd5d824661b05b5953bebe1064
Autor:
Tyler Kelley
Publikováno v:
Vetus Testamentum. 72:594-608
This study attempts to resolve some of the difficulties in understanding Zeph 2:1–3 by offering a holistic reading of the oracle presented in 1:2–2:3. It argues that the passage’s sacrificial imagery and the embedded polemic against the wealthy
Autor:
James S. Bullock, Andrew S. Graus, Tyler Kelley, Michael Boylan-Kolchin, Yuewen Qi, Shea Garrison-Kimmel
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 488:4585-4595
A standard prediction of galaxy formation theory is that the ionizing background suppresses galaxy formation in haloes with peak circular velocities smaller than Vpeak ~ 20 km/s, rendering the majority of haloes below this scale completely dark. We u
Autor:
Nick Zieser, Alina M. Zapalska, Michael S. Glinski, Tyler Kelley, Kim Young-McLear, Michael McCarty
Publikováno v:
Literacy Information and Computer Education Journal. 9:3002-3017
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 477:3164-3177
Winds are predicted to be ubiquitous in low-mass, actively star-forming galaxies. Observationally, winds have been detected in relatively few local dwarf galaxies, with even fewer constraints placed on their timescales. Here, we compare galactic outf
Publikováno v:
Problems and Perspectives in Management, Vol 14, Iss 1, Pp 30-43 (2016)
The paper presents specific examples of leadership training practices and educational activities that have been successfully implemented in an undergraduate program at the U.S. Coast Guard Academy. The purpose of this study is to illustrate a model o
Publikováno v:
Universal Journal of Educational Research. 4:426-431
As the National Science Foundation and engineers throughout the world seek to strengthen the future of the engineering profession, the Civil Engineering (CE) program at the United States Coast Guard Academy embodies this initiative with a student foc
Autor:
Shea Garrison-Kimmel, Andrew S. Graus, Tyler Kelley, Marcel S. Pawlowski, James S. Bullock, Michael Boylan-Kolchin
We introduce an extension of the ELVIS project to account for the effects of the Milky Way galaxy on its subhalo population. Our simulation suite, Phat ELVIS, consists of twelve high-resolution cosmological dark matter-only (DMO) zoom simulations of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::333bf4a121ad26ce85a71d3139dd1692
http://arxiv.org/abs/1811.12413
http://arxiv.org/abs/1811.12413
Autor:
Eliot Quataert, Claude André Faucher-Giguère, Andrew Wetzel, Tyler Kelley, Andrew S. Graus, Philip F. Hopkins, Shea Garrison-Kimmel, Robyn E. Sanderson, Michael Boylan-Kolchin, Dušan Kereš, James S. Bullock
Publikováno v:
Monthly Notices of the Royal Astronomical Society, vol 471, iss 2
Garrison-Kimmel, S; Wetzel, A; Bullock, JS; Hopkins, PF; Boylan-Kolchin, M; Faucher-Giguère, CA; et al.(2017). Not so lumpy after all: Modelling the depletion of dark matter subhaloes by Milky Way-like galaxies. Monthly Notices of the Royal Astronomical Society, 471(2), 1709-1727. doi: 10.1093/MNRAS/STX1710. UC Davis: Retrieved from: http://www.escholarship.org/uc/item/3pb4579b
NASA Astrophysics Data System
Garrison-Kimmel, S; Wetzel, A; Bullock, JS; Hopkins, PF; Boylan-Kolchin, M; Faucher-Giguère, CA; et al.(2017). Not so lumpy after all: Modelling the depletion of dark matter subhaloes by Milky Way-like galaxies. Monthly Notices of the Royal Astronomical Society, 471(2), 1709-1727. doi: 10.1093/MNRAS/STX1710. UC Davis: Retrieved from: http://www.escholarship.org/uc/item/3pb4579b
NASA Astrophysics Data System
Among the most important goals in cosmology is detecting and quantifying small ($M_{\rm halo}\simeq10^{6-9}~\mathrm{M}_\odot$) dark matter (DM) subhalos. Current probes around the Milky Way (MW) are most sensitive to such substructure within $\sim20$
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9473648f50fc308fe14a3a1c25151f4f
https://resolver.caltech.edu/CaltechAUTHORS:20170921-133516143
https://resolver.caltech.edu/CaltechAUTHORS:20170921-133516143
Publikováno v:
Interdisciplinary Education and Psychology. 1