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Akademický článek
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Akademický článek
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Autor:
Poghosyan, A. V., Pfau, W., Tsvetkova, K. P., Mugrauer, M., Tsvetkov, M. K., Hambaryan, V. V., Neuhaeuser, R., Kalaglarsky, D. G.
We present the archive of the wide-field plate observations obtained at the University Observatory Jena, which is stored at the Astrophysical Institute of the Friedrich Schiller University Jena. The archive contains plates taken in the period Februar
Externí odkaz:
http://arxiv.org/abs/1404.2401
Autor:
Tsvetkov, M., Milanova, M., Ivanova, I., Neov, D., Cherkezova-Zheleva, Z., Zaharieva, J., Abrashev, M.
Publikováno v:
In Journal of Molecular Structure 5 March 2019 1179:233-241
Autor:
Semkov, E. H., Peneva, S. P., Munari, U., Tsvetkov, M. K., Jurdana-Sepic, R., de Miguel, E., Schwartz, R. D., Dimitrov, D. P., Kjurkchieva, D. P., Radeva, V. S.
We present new results from optical photometric and spectroscopic observations of the eruptive pre-main sequence star V2493 Cyg (HBC 722). The object has continued to undergo significant brightness variations over the past few months and is an ideal
Externí odkaz:
http://arxiv.org/abs/1205.2532
Autor:
Elenkova D; Faculty of Chemistry and Pharmacy, Sofia University, 1164 Sofia, Bulgaria., Dimitrova Y; Faculty of Chemistry and Pharmacy, Sofia University, 1164 Sofia, Bulgaria., Tsvetkov M; Faculty of Chemistry and Pharmacy, Sofia University, 1164 Sofia, Bulgaria., Morgenstern B; Inorganic Solid State Chemistry, Saarland University, Campus Geb. C4 1, 66123 Saarbrücken, Germany., Milanova M; Faculty of Chemistry and Pharmacy, Sofia University, 1164 Sofia, Bulgaria., Todorovsky D; Faculty of Chemistry and Pharmacy, Sofia University, 1164 Sofia, Bulgaria., Zaharieva J; Faculty of Chemistry and Pharmacy, Sofia University, 1164 Sofia, Bulgaria.
Publikováno v:
Molecules (Basel, Switzerland) [Molecules] 2024 Aug 05; Vol. 29 (15). Date of Electronic Publication: 2024 Aug 05.
Autor:
Borrisov B; Institute of General and Inorganic Chemistry, Bulgarian Academy of Sciences, 11, Acad. G. Bonchev str., 1113 Sofia, Bulgaria., Tsvetkov M; Faculty of Chemistry and Pharmacy, Sofia University St. Kliment Ohridski, 1 James Bourchier blvd., 1164 Sofia, Bulgaria., Zahariev T; Institute of General and Inorganic Chemistry, Bulgarian Academy of Sciences, 11, Acad. G. Bonchev str., 1113 Sofia, Bulgaria., Elenkova D; Faculty of Chemistry and Pharmacy, Sofia University St. Kliment Ohridski, 1 James Bourchier blvd., 1164 Sofia, Bulgaria., Morgenstern B; Inorganic Solid State Chemistry, Saarland University, Campus Geb. C4 1, 66123 Saarbrücken, Germany., Dimov D; Institute of Optical Materials and Technologies, Bulgarian Academy of Sciences, 109, Acad. G. Bonchev str., 1113 Sofia, Bulgaria., Kukeva R; Institute of General and Inorganic Chemistry, Bulgarian Academy of Sciences, 11, Acad. G. Bonchev str., 1113 Sofia, Bulgaria., Trendafilova N; Institute of General and Inorganic Chemistry, Bulgarian Academy of Sciences, 11, Acad. G. Bonchev str., 1113 Sofia, Bulgaria., Georgieva I; Institute of General and Inorganic Chemistry, Bulgarian Academy of Sciences, 11, Acad. G. Bonchev str., 1113 Sofia, Bulgaria.
Publikováno v:
Inorganic chemistry [Inorg Chem] 2024 Jul 29; Vol. 63 (30), pp. 13840-13864. Date of Electronic Publication: 2024 Jul 12.
Publikováno v:
Open Chemistry, Vol 17, Iss 1, Pp 1124-1132 (2019)
The mixed metal oxides NiFe2O4 and Zn0.5Ni0.5Fe2O4 with a spinel-like structure, pure and modified with the lanthanide ions Eu(III) and Tb(III), were prepared by a sol-gel process in which propylene oxide was used as a gelling agent and then tested a
Externí odkaz:
https://doaj.org/article/53c8496fbdbb40a595c516735bf539f0
Saturated stellar images on digitised photographic plates are many times greater in area than the `seeing disk' seen in unsaturated CCD images. Indeed the flux profile of a bright star can be traced out for several degrees from the star's centre. The
Externí odkaz:
http://arxiv.org/abs/astro-ph/0502411
Publikováno v:
Mon.Not.Roy.Astron.Soc. 355 (2004) 591-600
We use the archive of the Bamberg Sky Patrol to obtain light curves of the active K subgiant CF Octantis for the interval 1964-1976. Digitised images of the field near CF Oct were obtained with a flat-bed scanner. Aperture photometry was performed of
Externí odkaz:
http://arxiv.org/abs/astro-ph/0409082