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166por Kubono, S, Teranishi, T, Notani, M, Yamaguchi, H, Saito, A, He, J J, Wakabayashi, M, Fujikawa, H, Amadio, G, Baba, H, Fukuchi, T, Shimoura, S, Michimasa, S, Nishimura, S, Nishimura, M, Gono, Y, Odahara, A, Kato, S, Moon, J Y, Lee, J H, Lee, C S, Kim, J C, Hahn, K I, Ishikawa, T, Hashimoto, T, Ishiyama, H, Watanabe, Y X, Tanaka, M H, Miyatake, H, Fülöp, Z S, Guimarães, V, Lichtenthäler, REnlace del recurso
Publicado 2004
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168
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169por Wallner, A, Bichler, M, Coquard, L, Dillmann, I, Forstner, O, Golser, R, Heil, M, Käppeler, F, Kutschera, W, Lederer-Woods, C, Martschini, M, Mengoni, A, Merchel, S, Michlmayr, L, Priller, A, Steier, P, Wiescher, M“…The neutron capture cross section of Be9 for stellar energies was measured via the activation technique using the Karlsruhe Van de Graaff accelerator in combination with accelerator mass spectrometry at the Vienna Environmental Research Accelerator. …”
Publicado 2019
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170por Zhao, Bo, Tomida, Kengo, Hennebelle, Patrick, Tobin, John J., Maury, Anaëlle, Hirota, Tomoya, Sánchez-Monge, Álvaro, Kuiper, Rolf, Rosen, Anna, Bhandare, Asmita, Padovani, Marco, Lee, Yueh-Ning“…We review recent progress in the formation and early evolution of disks around young stellar objects of both low-mass and high-mass, with an emphasis on mechanisms that may bridge the gap between observation and theory, including non-ideal MHD effects and asymmetric perturbations in the collapsing core (e.g., magnetic field misalignment and turbulence). …”
Publicado 2020
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Online Artículo Texto -
171por Tunes, Matheus A., Stemper, Lukas, Greaves, Graeme, Uggowitzer, Peter J., Pogatscher, Stefan“…The existing literature data shows that conventional aluminium alloys may not be suitable for use in stellar‐radiation environments as their hardening phases are prone to dissolve upon exposure to energetic irradiation, resulting in alloy softening which may reduce the lifetime of such materials impairing future human‐based space missions. …”
Publicado 2020
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172por Annunziatella, M., Biviano, A., Mercurio, A., Nonino, M., Rosati, P., Balestra, I., Presotto, V., Girardi, M., Gobat, R., Grillo, C., Medezinski, E., Kelson, D., Postman, M., Scodeggio, M., Brescia, M., Sartoris, B., Demarco, R., Fritz, A., Koekemoer, A., Lemze, D., Lombardi, M., Bradley, L., Coe, D., Donahue, M., Regös, E., Umetsu, K., Vanzella, E., Infante, L., Kuchner, U., Maier, C., Verdugo, M., Ziegler, B.“…The study of the galaxy stellar mass function (SMF) in relation to the galaxy environment and the stellar mass density profile, rho(r), is a powerful tool to constrain models of galaxy evolution. …”
Publicado 2014
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173
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174
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175
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177por Shaviv, Giora“…This beautifully illustrated book describes the birth and evolution of the theory of stellar structure through the vehement controversy between biology (as presented by Darwin) and physics (as presented by Kelvin) about the age of the Earth, which culminated with Rutherford suggesting radioactive dating. …”
Publicado 2009
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178por Goupil, Mariejo, Belkacem, Kévin, Neiner, Coralie, Lignières, Francois, Green, John“…Asteroseismology allows astrophysicists to test, to model and to understand stellar structure and evolution as never before. The chapters in this book address the two groups of topics summarized as "Stellar Rotation and Associated Seismology" as well as "Stellar Convection and Associated Seismology". …”
Publicado 2013
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