Zobrazeno 1 - 10
of 2 241
pro vyhledávání: '"Bode M"'
Autor:
Xin Zhou, Audrey Hilk, Norma V Solis, Nivea Pereira De Sa, Bode M Hogan, Tessa A Bierbaum, Maurizio Del Poeta, Scott G Filler, Laura S Burrack, Anna Selmecki
Publikováno v:
PLoS Pathogens, Vol 20, Iss 7, p e1012389 (2024)
Ergosterol is essential for fungal cell membrane integrity and growth, and numerous antifungal drugs target ergosterol. Inactivation or modification of ergosterol biosynthetic genes can lead to changes in antifungal drug susceptibility, filamentation
Externí odkaz:
https://doaj.org/article/74e7071a7fd741f9867c94874908f19c
Autor:
Zamanov, R. K., Stoyanov, K. A., Marchev, V., Minev, M., Marchev, D., Moyseev, M., Marti, J., Bode, M. F., Konstantinova-Antova, R., Stefanov, S.
We present high resolution (0.06 A/px) spectroscopic observations of the recurrent nova T Coronae Borealis obtained during the last 1.5 years (September 2022 -- January 2024), with the 2.0m RCC telecope of the Rozhen National Astronomical Observatory
Externí odkaz:
http://arxiv.org/abs/2405.11506
Autor:
Zamanov, R., Boeva, S., Latev, G. Y., Semkov, E., Minev, M., Kostov, A., Bode, M. F., Marchev, V., Marchev, D.
Context: T CrB (NOVA CrB 1946) is a famous recurrent nova with a recurrence timescale of 80 years. Aims: We aim to estimate the colours, luminosity, and mass-accretion rate for T CrB (NOVA CrB 1946) during and after the superactive state. Methods and
Externí odkaz:
http://arxiv.org/abs/2312.04342
Publikováno v:
Current Directions in Biomedical Engineering, Vol 1, Iss 1, Pp 524-528 (2015)
One of the major challenges in developing appropriate vascular substitutes is to produce a graft that adapts to the biological and mechanical conditions at the application or implantation site. One approach is the use of tissue engineered electrospun
Externí odkaz:
https://doaj.org/article/1d8321359fbd4bb8872338e2868b5dce
The Be stars display variable optical emission lines originating in the circumstellar disc. Here we analyse high resolution spectroscopic observations of Be stars and the distance between the peaks of H-alpha, H-beta, and H-gamma emission lines ($\De
Externí odkaz:
http://arxiv.org/abs/2302.11975
High Resolution X-ray Spectra of RS Ophiuchi (2006 and 2021): Revealing the cause of SSS variability
Autor:
Ness, J. -U., Beardmore, A. P., Bode, M. F., Darnley, M. J., Dobrotka, A., Drake, J. J., Magdolen, J., Munari, U., Osborne, J. P., Orio, M., Page, K. L., Starrfield, S.
Publikováno v:
A&A 670, A131 (2023)
Swift observed the SSS phase in RS Oph much fainter in 2021 than in 2006, and we compare an XMM-Newton grating spectrum on day 55.6 in 2021 (2021d55.6) to SSS Chandra and XMM-Newton grating spectra from days 2006d39.7, 2006d54, and 2006d66.9. We pres
Externí odkaz:
http://arxiv.org/abs/2212.07169
Autor:
Zamanov, R. K., Kostov, A., Moyseev, M., Petrov, N., Nikolov, Y. M., Latev, G. Y., Marchev, D., Boeva, S., Stoyanov, K. A., Minev, M. S., Marti, J., Radeva, V., Sanchez-Ayaso, E., Bode, M. F., Ilkiewicz, K., Nikolov, G., Luque-Escamilla, P. L., Spassov, B., Borisov, B., Marchev, V. D., Kurtenkov, A.
We report photometric observations of the hidden symbiotic star SU Lyn in the optical bands. In five nights we detect a weak flickering in U band with amplitude of about 0.05 magnitudes. No intranight variations are found in B, V, g' and r' bands. Th
Externí odkaz:
http://arxiv.org/abs/2206.10151
Autor:
Zamanov, R. K., Stoyanov, K. A., Marchev, D., Tomov, N. A., Wolter, U., Bode, M. F., Nikolov, Y. M., Stefanov, S. Y., Kurtenkov, A., Latev, G. Y.
We present new spectroscopic observations of the Be/black hole binary MWC 656 obtained during the period 2015 - 2021. We measure the equivalent width of H$\alpha$ (EW$_\alpha$), H$\beta$ ($EW_\beta$), and the distance between the peaks of H$\alpha$ (
Externí odkaz:
http://arxiv.org/abs/2206.06013
Autor:
Page, K. L., Beardmore, A. P., Osborne, J. P., Munari, U., Ness, J. -U., Evans, P. A., Bode, M. F., Darnley, M. J., Drake, J. J., Kuin, N. P. M., O'Brien, T. J., Orio, M., Shore, S. N., Starrfield, S., Woodward, C. E.
On 2021 August 8, the recurrent nova RS Ophiuchi erupted again, after an interval of 15.5 yr. Regular monitoring by the Neil Gehrels Swift Observatory began promptly, on August 9.9 (0.37 day after the optical peak), and continued until the source pas
Externí odkaz:
http://arxiv.org/abs/2205.03232
Autor:
Pfnür, H., Tegenkamp, C., Sanna, S., Jeckelmann, E., Horn-von Hoegen, M., Bovensiepen, U., Esser, N., Schmidt, W.G., Dähne, M., Wippermann, S., Bechstedt, F., Bode, M., Claessen, R., Ernstorfer, R., Hogan, C., Ligges, M., Pucci, A., Schäfer, J., Speiser, E., Wolf, M., Wollschläger, J.
Publikováno v:
In Surface Science Reports May 2024 79(2)