Zobrazeno 1 - 10
of 46
pro vyhledávání: '"A. S. Kudashkina"'
Publikováno v:
Вестник рентгенологии и радиологии, Vol 104, Iss 4, Pp 244-254 (2024)
Background. Pancreatic head cancer ranks 6–7th among oncologic diseases and 4–5th among causes of mortality, with only 5% of patients achieving 5-year survival rate to date. Despite the successes of modern diagnostics and surgical treatment, the
Externí odkaz:
https://doaj.org/article/594d250cd00449c0a95dcb840dc6f5a8
Autor:
A. P. Polyakov, L. V. Bolotina, A. L. Kornietskaya, D. S. Kudashkina, D. V. Sidorov, A. A. Troitskiy, A. R. Gevorkov
Publikováno v:
Опухоли головы и шеи, Vol 12, Iss 1, Pp 114-119 (2022)
Cutaneous melanoma is characterized by an aggressive course associated with a tendency to metastasis. For a long time, the prognosis of patients with metastatic melanoma remained extremely poor. However, the introduction of immunooncological drugs in
Externí odkaz:
https://doaj.org/article/ea24c848bd484110b4f97cd901fa2716
Autor:
L. S. Kudashkina
Publikováno v:
Odessa Astronomical Publications, Vol 33, Iss 0, Pp 34-39 (2020)
For the group of pulsating variable stars with multi-component variability – which are currently classified as the RV Tau-type stars – the classification based on complexity of the periodograms is discussed. Per- iodograms were computed using the
Externí odkaz:
https://doaj.org/article/14cc97e4be8f434d85332b494a5937cf
Autor:
L. S. Kudashkina, I. L. Andronov
Publikováno v:
Odessa Astronomical Publications, Vol 30, Iss 0, Pp 93-97 (2017)
Using the phase plane diagrams, the phase light curves of a group of the Mira-type stars and semi-regular variables are analyzed. As generalized coordinates х and ẋ, we have used m – the brightness of the star and its phase derivative. We have u
Externí odkaz:
https://doaj.org/article/f1d5c9bbc9354d8b83c9cfb59f5e6d4e
Autor:
L. S. Kudashkina, I. L. Andronov
Publikováno v:
Odessa Astronomical Publications, Vol 9, Iss 0, Pp 108-111 (2017)
For 62 Mira-type stars the values of periods have been redetermined; the mean curves have been fitted by a trigonometric polynomial with an optimal number of harmonics; a number of the parameters of the light curve have been calculated (amplitude of
Externí odkaz:
https://doaj.org/article/1bb109d5ab2b4b6d8b27958055ae766e
Autor:
L. S. Kudashkina, G. M. Rudnitskij
Publikováno v:
Odessa Astronomical Publications, Vol 7, Iss 1, Pp 66-69 (2017)
The shapes of light curves of Mira-type variable stars is analyzed. It is shown that some features of the light curves may be explained by passage of shock waves in the stars' atmospheres. In particular, it is noted that "steps" of the ascending bran
Externí odkaz:
https://doaj.org/article/8ae0a855b2304649bf3ef74e9493097b
Autor:
Yu. S. Efimov, L. S. Kudashkina
Publikováno v:
Odessa Astronomical Publications, Vol 14, Iss 0, Pp 134-139 (2017)
The variations of the polarization parameters of three Mira-type stars V CrB, S CrB, T Her in the UBVRI bands are presented.
Externí odkaz:
https://doaj.org/article/94787151cc27409394f9b9f08d7061d8
Autor:
I. V. Arutyunyan, A. G. Soboleva, K. B. Gordon, D. S. Kudashkina, D. A. Miroshnichenko, A. P. Polyakov, I. V. Rebrikova, A. V. Makarov, A. V. Lokhonina, T. Kh. Fatkhudinov
Publikováno v:
Bulletin of Experimental Biology and Medicine. 173:553-559
Autor:
L. S. Kudashkina
Publikováno v:
Odessa Astronomical Publications, Vol 29, Iss 0, Pp 78-81 (2016)
. For nine Mira-type stars (o Cet, R Leo, S Car, U Her, X Oph, R Aql, RR Aql, S Ori, S Scl,) and one semi-regular star (L2 Pup), the mean light curves have been obtained. The initial values of the brightness (observations) were fitted by a trigonomet
Externí odkaz:
https://doaj.org/article/6fa60c03bf914743b700dd164135ed9b
Autor:
I. L. Andronov, L. L. Chinarova, V. F. Gopka, E. V. Menchenkova (Luthardt), M. I. Myalkovskij, M. P. Kosmykina (Yasinskaya), L. S. Kudashkina, A. V. Yushchenko
Publikováno v:
Odessa Astronomical Publications, Vol 9, Iss 0 (2017)
The work of the Odessa Correspondence Courses is briefly described.
Externí odkaz:
https://doaj.org/article/c12e4512fb724eb6b9d03a8ac835eb3e