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pro vyhledávání: '"Holmberg J"'
Comparing physical protection strategies against insider threats using probabilistic risk assessment
Publikováno v:
In Nuclear Engineering and Design May 2022 391
Autor:
Hosseini, S.B., Mallipeddi, D., Holmberg, J., Rännar, L.-E., Koptyug, A., Sjöström, W., Krajnik, P., Klement, U.
Publikováno v:
In Procedia CIRP 2022 115:72-77
Autor:
Kokkirala, S., Osman, K., Holmberg, J., Kimming, S., Iwasaki, H., Klement, U., Hosseini, S.B.
Publikováno v:
Procedia CIRP; 2024, Vol. 123, p292-297, 6p
Autor:
Casagrande, L., Portinari, L., Glass, I. S., Laney, D., Aguirre, V. Silva, Datson, J., Andersen, J., Nordström, B., Holmberg, J., Flynn, C., Asplund, M.
Publikováno v:
2014, MNRAS, 439, 2060
The apparent size of stars is a crucial benchmark for fundamental stellar properties such as effective temperatures, radii and surface gravities. While interferometric measurements of stellar angular diameters are the most direct method to gauge thes
Externí odkaz:
http://arxiv.org/abs/1401.3754
The existence of a kinematically defined moving group of stars centred at U = -40, V = -17 km/s referred to as the Hyades Supercluster, has been suggested as the debris of an originally large star forming event, with its core being the present day Hy
Externí odkaz:
http://arxiv.org/abs/1103.2588
Ages, chemical compositions, velocity vectors, and Galactic orbits for stars in the solar neighbourhood are fundamental test data for models of Galactic evolution. We aim to improve the accuracy of the Geneva-Copenhagen Survey data by implementing th
Externí odkaz:
http://arxiv.org/abs/0811.3982
Akademický článek
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Ages, metallicities, space velocities, and Galactic orbits of stars in the Solar neighbourhood are fundamental observational constraints on models of galactic disk evolution. We aim to consolidate the calibrations of uvby photometry into Te, [Fe/H],
Externí odkaz:
http://arxiv.org/abs/0707.1891
Here, we present our on-going work on the determination of stellar parameters of giants in the Galactic Disks and Bulge observed with UVES on the VLT. We present some preliminarily results.
Comment: 2 pages, IAU241 conference proceedings
Comment: 2 pages, IAU241 conference proceedings
Externí odkaz:
http://arxiv.org/abs/astro-ph/0701913
Autor:
Bersier, D., Fruchter, A. S., Strolger, L. -G., Gorosabel, J., Levan, A., Burud, I., Rhoads, J. E., Becker, A. C., Cassan, A., Chornock, R., Covino, S., de Jong, R. S., Dominis, D., Filippenko, A. V., Hjorth, J., Holmberg, J., Malesani, D., Mobasher, B., Olsen, K. A. G., Stefanon, M., Cerón, J. M. Castro, Fynbo, J. P. U., Holland, S. T., Kouveliotou, C., Pedersen, H., Tanvir, N. R., Woosley, S. E.
Publikováno v:
Astrophys.J.643:284-291,2006
We present ground-based and Hubble Space Telescope optical observations of the X-ray flash (XRF) 020903, covering 300 days. The afterglow showed a very rapid rise in the first day, followed by a relatively slow decay in the next few days. There was a
Externí odkaz:
http://arxiv.org/abs/astro-ph/0602163