Zobrazeno 1 - 10
of 1 394
pro vyhledávání: '"Durán, S"'
Autor:
Moreno-Estébanez, A., Marinas, A., Garamendi Ruiz, I., González Eizaguirre, A., Reurich-Gómez, N., Boyero Durán, S., Mendibe Bilbao, M.M., Rodríguez-Antigüedad, A.
Publikováno v:
In Neurology Perspectives January-March 2024 4(1)
Publikováno v:
Acta Ortopédica Mexicana. sep/oct2023, Vol. 37 Issue 5, p270-275. 6p.
Autor:
Cabezas, R., Duran, S., Zurob, E., Plaza, A., Merlet, G., Araya-Lopez, C., Romero, J., Quijada-Maldonado, E.
Publikováno v:
In Journal of Membrane Science 1 November 2021 637
Autor:
René F. Cárdenas, Rosalía Durán S., Francisco Ceballos E., Jaime Plaza C., Jaime Sánchez S., Elfa Haro S.
Publikováno v:
Oncología, Vol 12, Iss 3-4 (2022)
Se presenta una revisión del tema del uso de la gammagrafía mamaria mediante 99mTc-sestamibi tanto en la etapa del manejo diagnóstico inicial, como en el valor de este proceder como indicador de la actividad funcional del sistema de resistencia a
Externí odkaz:
https://doaj.org/article/64dae6d7f6c84301bc09b92899d40c6b
Autor:
Gokce, E. Yaz, Karaali, S., Duran, S., Bilir, S., Yalcinkaya, A., Ak, S., Ak, T., Lopez-Corredoira, M., Cabrera-Lavers, A.
We estimated the scale-length of the thin disc with the J and W1 magnitudes of the most probable Red Clump (RC) stars in the Galactic plane, $-0\overset{^\circ}.5 \leq b \leq +0\overset{^\circ}.5$, in 19 equal sized fields with consecutive Galactic l
Externí odkaz:
http://arxiv.org/abs/1503.01781
Autor:
Cárdenas Fernández, MC., Pérez Surribas, D., Pérez Garay, R., Jiménez Jiménez, J., Gella Concustell, A., Zapico Muñiz, E., Cruz Iglesias, E., Fernández García, M., Hermoso Durán, S., Marcaida Benito, G., Valldecabres Ortiz, C.
Publikováno v:
In Clinica Chimica Acta November 2020 510:573-580
Akademický článek
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Autor:
Yontan, T., Bilir, S., Bostancı, Z. F., Ak, T., Karaali, S., Güver, T., Ak, S., Duran, S., Paunzen, E.
We present the results of CCD UBVRI observations of the open cluster NGC 6811 obtained on 18th July 2012 with the 1m telescope at the T\"UB\.ITAK National Observatory (TUG). Using these photometric results, we determine the structural and astrophysic
Externí odkaz:
http://arxiv.org/abs/1410.3129
By measuring precise radial velocities of planetary nebulae (which belong to the intermediate age population), H II regions, and A-type supergiant stars (which are members of the young population) in NGC 6822, we aim to determine if both types of pop
Externí odkaz:
http://arxiv.org/abs/1405.5519
Autor:
Ak, S., Ak, T., Karaali, S., Bilir, S., Guctekin, S. Tuncel, Tas, O. Onal, Ozturkmen, N. D., Duran, S., Coskunoglu, B., Yontan, T., Gokce, E. Yaz, Eker, Z.
The transformation equations from $BVR_c$ to $g'r'i'$ magnitudes and vice versa for the giants were established from a sample of 80 stars collected from Soubiran et al. (2010) with confirmed surface gravity ($2\leq \log g$ (cms$^{-2}$)$ \leq3$) at ef
Externí odkaz:
http://arxiv.org/abs/1401.5479