Zobrazeno 1 - 10
of 1 891
pro vyhledávání: '"Racz M"'
Publikováno v:
IBVS, 6089, 1, 2014
We examine the long-term light curve, optical spectrum, spectral energy distribution, and Galactic location of V1117 Her in order to establish its nature. V1117 Her is most probably a young intermediate-mass star whose cyclic brightness dimmings are
Externí odkaz:
http://arxiv.org/abs/1401.1952
Autor:
Kun, M., Szegedi-Elek, E., Moór, A., Ábrahám, P., Acosta-Pulido, J. A., Apai, D., Kelemen, J., Pál, A., Rácz, M., Regály, Zs., Szakáts, R., Szalai, N., Szing, A.
We conducted a long-term optical photometric and spectroscopic monitoring of the strongly variable, accreting young sun-like star [KOS94] HA11, associated with the dark cloud Lynds 1340, that exhibited large amplitude (5-6 magnitudes in the I_C band)
Externí odkaz:
http://arxiv.org/abs/1104.2428
Autor:
Kun, M., Szegedi-Elek, E., Moór, A., Kóspál, Á., Ábrahám, P., Apai, D., Kiss, Z. T., Klagyivik, P., Magakian, T. Yu., Mező, Gy., Movsessian, T. A., Pál, A., Rácz, M., Rogers, J.
Young Sun-like stars at the beginning of the pre-main sequence (PMS) evolution are surrounded by accretion discs and remnant protostellar envelopes. Photometric and spectroscopic variations of these stars are driven by interactions of the star with t
Externí odkaz:
http://arxiv.org/abs/1101.2329
Autor:
Vinko, J., Takats, K., Sarneczky, K., Szabo, Gy. M., Meszaros, Sz., Csorvasi, R., Szalai, T., Gaspar, A., Pal, A., Csizmadia, Sz., Kospal, A., Racz, M., Kun, M., Csak, B., Furesz, G., DeBond, H., Grunhut, J., Thomson, J., Mochnacki, S., Koktay, T.
Publikováno v:
Mon.Not.Roy.Astron.Soc.369:1780-1796,2006
New BVRI photometry and optical spectroscopy of the Type IIp supernova 2004dj in NGC 2403, obtained during the first year since discovery, are presented. The progenitor cluster, Sandage 96, is also detected on pre-explosion frames. The light curve in
Externí odkaz:
http://arxiv.org/abs/astro-ph/0604230
V1647 Ori is a young eruptive star, which went into outburst at the end of 2003. Since then, the object is gradually fading. In October 2005, however, V1647 Ori started a very rapid fading, approximately 1 mag/month in I_C as opposed to 0.1 mag/month
Externí odkaz:
http://arxiv.org/abs/astro-ph/0511733
Autor:
Acosta-Pulido, J. A., Kun, M., Abraham, P., Kospal, A., Csizmadia, Sz., Kiss, L. L., Moor, A., Szabados, L., Benko, J. M., Delgado, R. Barrena, Charcos-Llorens, M., Eredics, M., Kiss, Z. T., Manchado, A., Racz, M., Ramos-Almeida, C., Szekely, P., Vidal-Nunez, M. J.
(Abridged) We studied the brightness and spectral evolution of the young eruptive star V1647 Ori during its recent outburst in the period 2004 February - 2006 Sep. We performed a photometric follow-up in the bands V, R_C, I_C, J, H, K_s as well as vi
Externí odkaz:
http://arxiv.org/abs/astro-ph/0408432
Akademický článek
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Autor:
S. B. Lucas
Publikováno v:
The Journal of Pathology. 164:92-92
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::269c46c16403ca607d00203a94757488
https://doi.org/10.1002/path.1711640119
https://doi.org/10.1002/path.1711640119
Autor:
Lee MJ; Department of Infectious Disease, Imperial College London, UK., Godakandaarachchi P; Harrison Wing, Department of HIV, Guy's and St Thomas Hospital NHS Foundation Trust, UK., Collins S; HIV I-Base, UK., Racz M; Harrison Wing, Department of HIV, Guy's and St Thomas Hospital NHS Foundation Trust, UK., Sharp A; Harrison Wing, Department of HIV, Guy's and St Thomas Hospital NHS Foundation Trust, UK., Fidler S; Department of Infectious Disease, Imperial College London, UK., Fox J; Harrison Wing, Department of HIV, Guy's and St Thomas Hospital NHS Foundation Trust, UK.
Publikováno v:
Journal of virus eradication [J Virus Erad] 2023 Dec 15; Vol. 9 (4), pp. 100360. Date of Electronic Publication: 2023 Dec 15 (Print Publication: 2023).
Publikováno v:
European Journal of Epidemiology, 1988 Sep 01. 4(3), 382-385.
Externí odkaz:
https://www.jstor.org/stable/3520936