Zobrazeno 1 - 10
of 330
pro vyhledávání: '"Nesvacil N."'
Autor:
Tan, L.T., Tanderup, K., Nappa, A., Petric, P., Jürgenliemk-Schulz, I.M., Serban, M., Swamidas, J.V., Palmu, M., Duke, S.L., Mahantshetty, U., Nesvacil, N., Pötter, R.C., Nout, R.A.
Publikováno v:
In Clinical and Translational Radiation Oncology July 2021 29:85-92
Autor:
Knoth, J., Sturdza, A., Zaharie, A., Dick, V., Kronreif, G., Nesvacil, N., Widder, J., Kirisits, C., Schmid, M. P
Publikováno v:
Strahlentherapie und Onkologie; Aug2024, Vol. 200 Issue 8, p684-690, 7p
Autor:
Knoth, J., Pötter, R., Jürgenliemk-Schulz, I.M., Haie-Meder, C., Fokdal, L., Sturdza, A., Hoskin, P., Mahantshetty, U., Segedin, B., Bruheim, K., Wiebe, E., Rai, B., Cooper, R., van der Steen-Banasik, E., van Limbergen, E., Pieters, B.R., Sundset, M., Tan, L.T., Nout, R.A., Tanderup, K., Kirisits, C., Nesvacil, N., Lindegaard, J.C., Schmid, M.P.
Publikováno v:
In Gynecologic Oncology October 2020 159(1):136-141
Autor:
Nesvacil, N., Lüftinger, T., Shulyak, D., Obbrugger, M., Weiss, W., Drake, N. A., Hubrig, S., Ryabchikova, T., Kochukhov, O., Piskunov, N., Polosukhina, N.
In atmospheres of magnetic main-sequence stars, the diffusion of chemical elements leads to a number of observed anomalies, such as abundance spots across the stellar surface. The aim of this study was to derive a detailed picture of the surface abun
Externí odkaz:
http://arxiv.org/abs/1303.2703
Autor:
Lüftinger, T., Fröhlich, H. -E., Weiss, W., Petit, P., Aurière, M., Nesvacil, N., Gruberbauer, M., Shulyak, D., Alecian, E., Baglin, A., Baudin, F., Catala, C., Donati, J. -F., Kochukhov, O., Michel, E., Piskunov, N., Roudier, T., Samadi, R.
We compare surface maps of the chemically peculiar star HD 50773 produced with a Bayesian technique and based on high quality CoRoT photometry with those derived from rotation phase resolved spectropolarimetry. The goal is to investigate the correlat
Externí odkaz:
http://arxiv.org/abs/0911.3791
The 5.9 M_sun star HD 125823 is a striking helium variable with a period of 8.82 d, ranging in helium spectral type from He-strong B2 to He-weak B8. For the first time we present here observational evidence for the appearance of emission lines of Mn
Externí odkaz:
http://arxiv.org/abs/astro-ph/0703478
Autor:
Hubrig, S., Nesvacil, N.
Publikováno v:
Mon.Not.Roy.Astron.Soc.Lett.378:L16-L19,2007
We report the discovery of resolved magnetically split lines in two chemically peculiar stars, the SrEuCr star HD 92499 and the Bp SiCr star HD 157751. From FEROS spectra, we have measured a mean magnetic field modulus of 8.5 kG for HD 92499 and a me
Externí odkaz:
http://arxiv.org/abs/astro-ph/0703228
Using recent spectroscopic observations, we show that the triple system AO Vel with an eclipsing BpSi primary is in fact a remarkable quadruple system formed by two double-lined spectroscopic binaries with components close to the ZAMS. All available
Externí odkaz:
http://arxiv.org/abs/astro-ph/0512511
Autor:
Solano, E., Catala, C., Garrido, R., Poretti, E., Janot-Pacheco, E., Gutierrez, R., Gonzalez, R., Mantegazza, L., Neiner, C., Fremat, Y., Charpinet, S., Weiss, W., Amado, P. J., Rainer, M., Tsymbal, V., Lyashko, D., Ballereau, D., Bouret, J. C., Hua, T., Katz, D., Lignieres, F., Luftinger, T., Mittermayer, P., Nesvacil, N., Soubiran, C., Veer-Menneret, C. Van't, Goupil, M. J., Costa, V., Rolland, A., Antonello, E., Bossi, M., Buzzoni, A., Rodrigo, C., Aerts, C., Butler, C. J., Guenther, E., Hatzes, A.
The GAUDI database (Ground-based Asteroseismology Uniform Database Interface, http://sdc.laeff.esa.es/gaudi/) is a preparatory archive for the COROT (COnvection, ROtation and planetary Transits, http://www.astrsp-mrs.fr/projets/corot/) mission develo
Externí odkaz:
http://arxiv.org/abs/astro-ph/0409748
Publikováno v:
Commun.Asteros. 144 (2004) 43-78
NEMO.2003 (vienna NEw MOdel grid of stellar atmospheres) is a DVD with 91,520 stellar model atmospheres representing a 5D grid of modified ATLAS9 atmospheres; the purpose of the modifications was to include different treatments of convection and high
Externí odkaz:
http://arxiv.org/abs/astro-ph/0406381