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Akademický článek

J. G. L. Prior MB, BS, FFARCS

Publikováno v: British Medical Journal (Clinical Research Edition), 1983 Apr . 286(6375), 1451-1451.

Externí odkaz: https://www.jstor.org/stable/29510792

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The early evolution of young massive clusters: The kinematic history of NGC6611 / M16

Autor: Stoop, Mitchel, Kaper, Lex, de Koter, Alex, Guo, Difeng, Lamers, Henny J. G. L. M., Rieder, Steven

Publikováno v: A&A 670, A108 (2023)

In the first few Myr the massive stars dynamically interact, produce runaways and affect the initial binary population. Observing and interpreting the dynamics of young massive clusters is key to our understanding of the star formation process and pr

Externí odkaz: http://arxiv.org/abs/2207.08452

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Quantum jump simulation in three-level systems using photonic Gaussian modes

Autor: Cardoso, A. C., Condé, J. G. L., Marques, B., Cabral, J. S., Pádua, S.

Publikováno v: Phys. Rev. A 103, 013722 (2021)

Multi-level quantum systems loose coherence due to quantum jumps or spontaneous decay between their internal levels. Here we propose a way to simulate experimentally a three-level system under quantum jump using a three-mode photonic system. We simul

Externí odkaz: http://arxiv.org/abs/2006.06144

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Akademický článek

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Akademický článek

Mass-loss rates and the mass evolution of star clusters H. J. G. L. M. Lamers, H. Baumgardt and M. Gieles Mass loss and the evolution of star clusters.

Autor: Lamers, Henny J. G. L. M.¹ lamers@astro.uu.nl, Baumgardt, Holger^2,3 h.baumgardt@uq.edu.au, Gieles, Mark^4,5 mgieles@ast.cam.ac.uk

Publikováno v: Monthly Notices of the Royal Astronomical Society. Nov2010, Vol. 409 Issue 1, p305-328. 24p. 4 Charts, 17 Graphs.

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The difference in metallicity distribution functions of halo stars and globular clusters as a function of galaxy type: A tracer of globular cluster formation and evolution

Autor: Lamers, Henny J. G. L. M., Kruijssen, J. M. Diederik, Bastian, Nate, Rejkuba, Marina, Hilker, Michael, Kissler-Patig, Markus

Observations of globular clusters (GCs) and field stars in the halos of the giant elliptical galaxy Cen A and the spiral galaxy M31 show a large range of cluster-to-star number ratios ('specific frequencies'). The cluster-to-star ratio decreases with

Externí odkaz: http://arxiv.org/abs/1706.00939

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