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pro vyhledávání: '"I A, Carlo"'
Context: The formation of rocky planetesimals is a long-standing problem in planet formation theory. One of the possibilities is that it results from gravitational instability as a result of pile-up of small silicate dust particles released from subl
Externí odkaz:
http://arxiv.org/abs/2011.13164
Autor:
Jess, David B., Dillon, Chris J., Kirk, Michael S., Reale, Fabio, Mathioudakis, Mihalis, Grant, Samuel D. T., Christian, Damian J., Keys, Peter H., Prasad, S. Krishna, Houston, Scott J.
Small-scale magnetic reconnection processes, in the form of nanoflares, have become increasingly hypothesized as important mechanisms for the heating of the solar atmosphere, for driving propagating disturbances along magnetic field lines in the Sun'
Externí odkaz:
http://arxiv.org/abs/1812.06978
Publikováno v:
In Physica Medica November 2019 67:1-8
Publikováno v:
In Applied Radiation and Isotopes April 2017 122:193-201
Autor:
Longland, Richard, Iliadis, Christian, Champagne, Art, Newton, Joe, Ugalde, Claudio, Coc, Alain, Fitzgerald, Ryan
A method based on Monte Carlo techniques is presented for evaluating thermonuclear reaction rates. We begin by reviewing commonly applied procedures and point out that reaction rates that have been reported up to now in the literature have no rigorou
Externí odkaz:
http://arxiv.org/abs/1004.4136
The anomalous X-ray pulsars and soft gamma-repeaters are peculiar high-energy sources believed to host a magnetar, i.e. an ultra-magnetized neutron star. Their persistent, soft X-ray emission (~1-10 keV)is usually modeled by the superposition of a bl
Externí odkaz:
http://arxiv.org/abs/0802.2647
Anisotropic Galactic Outflows and Enrichment of the Intergalactic Medium. I: Monte Carlo Simulations
We have developed an analytical model to describe the evolution of anisotropic galactic outflows. With it, we investigate the impact of varying opening angle on galaxy formation and the evolution of the IGM. We have implemented this model in a Monte
Externí odkaz:
http://arxiv.org/abs/astro-ph/0606423
Akademický článek
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Autor:
Burgasser, Adam J.
Publikováno v:
Astrophys.J.Suppl.155:191-207,2004
Monte Carlo simulations of the field substellar mass function (MF) are presented. Starting from various representations of the MF below 0.1 M$_{\sun}$ and the stellar birth rate, luminosity functions (LFs) and T$_{eff}$ distributions are produced for
Externí odkaz:
http://arxiv.org/abs/astro-ph/0407624
Autor:
Kim, Rita S. J., Kepner, Jeremy V., Postman, Marc, Strauss, Michael A., Bahcall, Neta A., Gunn, James E., Lupton, Robert H., Annis, James, Nichol, Robert C., Castander, Francisco J., Brinkmann, J., Brunner, Robert J., Connolly, Andrew, Csabai, Istvan, Hindsley, Robert B., Ivezic, Zeljko, Vogeley, Michael S., York, Donald G.
Publikováno v:
Astron.J.123:20-36,2002
We present a comparison of three cluster finding algorithms from imaging data using Monte Carlo simulations of clusters embedded in a 25 deg^2 region of Sloan Digital Sky Survey (SDSS) imaging data: the Matched Filter (MF; Postman et al. 1996), the A
Externí odkaz:
http://arxiv.org/abs/astro-ph/0110259