Zobrazeno 1 - 10
of 2 164
pro vyhledávání: '"Hussain G"'
Autor:
Abubaker M Hamad, Rania Mahjoub Ser Alkhatem, Asaad K Algahany, Hussain G Ahmed, Abdulaziz Alfahed, Hisham Ali Waggiallah
Publikováno v:
International Journal of Biomedicine, Vol 13, Iss 1, Pp 62-68 (2023)
The goal of our study was to determine the expression and phosphorylation of PTEN at residues Ser380/Thr382/383, as well as the nuclear expression of p53 in Sudanese patients with breast cancer (BC) in association with clinicopathological aspects of
Externí odkaz:
https://doaj.org/article/f7c856ef020c4222821317e5c272b63d
Autor:
Hend M Alkwai, Amany M Khalifa, Ahmed M Ahmed, Alfatih M Alnajib, Khaznah A Alshammari, Muslima M Alrashidi, Hussain G Ahmed
Publikováno v:
SAGE Open Medicine, Vol 10 (2022)
A substantial number of COVID-19 survivors describe ongoing symptoms long after the acute phase. This so-called post-COVID-19 syndrome or long COVID occurs irrespective of initial disease severity. Objectives: This cross-sectional study aims to descr
Externí odkaz:
https://doaj.org/article/4728b206dd9d445085f5024b643e7fc3
Autor:
Bellotti, S., Evensberget, D., Vidotto, A. A., Lavail, A., Lueftinger, T., Hussain, G. A. J., Morin, J., Petit, P., Saikia, S. Boro, Danielski, C., Micela, G.
The accurate characterisation of the stellar magnetism of planetary host stars has been gaining momentum, especially in the context of transmission spectroscopy investigations of exoplanets. Indeed, the magnetic field regulates the amount of energeti
Externí odkaz:
http://arxiv.org/abs/2405.19052
We present a multiwavelength study of AB Doradus, combining modelling that incorporates a spectropolarimetric magnetic field map with 8.4 GHz radio interferometry to measure the coronal extent and density of this young star. We use the surface magnet
Externí odkaz:
http://arxiv.org/abs/2404.06304
Autor:
Bellotti, S., Morin, J., Lehmann, L. T., Petit, P., Hussain, G. A. J., Donati, J. -F., Folsom, C. P., Carmona, A., Martioli, E., Klein, B., Fouque, P., Moutou, C., Alencar, S., Artigau, E., Boisse, I., Bouchy, F., Bouvier, J., Cook, N. J., Delfosse, X., Doyon, R., Hebrard, G.
Dynamo models of stellar magnetic fields for partly and fully convective stars are guided by observational constraints. Zeeman-Doppler imaging has revealed a variety of magnetic field geometries and, for fully convective stars in particular, a dichot
Externí odkaz:
http://arxiv.org/abs/2403.08590
We aim to characterise the magnetic field of the eclipsing binary CU Cnc. The determination of magnetic field parameters of this target enables comparisons with both observations of similar stars and theoretical predictions of the magnetic field stre
Externí odkaz:
http://arxiv.org/abs/2402.00721
Autor:
Tsvetkova, S., Morin, J., Folsom, C. P., Bouquin, J. -B. Le, Alecian, E., Bellotti, S., Hussain, G., Kochukhov, O., Marsden, S. C., Neiner, C., Petit, P., Wade, G. A., collaboration, the BinaMIcS
This work is part of the BinaMIcS project, the aim of which is to understand the interaction between binarity and magnetism in close binary systems. All the studied spectroscopic binaries targeted by the BinaMIcS project encompass hot massive and int
Externí odkaz:
http://arxiv.org/abs/2312.04247
Autor:
Vidotto, A. A., Bourrier, V., Fares, R., Bellotti, S., Donati, J. F., Petit, P., Hussain, G. A. J., Morin, J.
Publikováno v:
A&A 678, A152 (2023)
The M dwarf star GJ 436 hosts a warm-Neptune that is losing substantial amount of atmosphere, which is then shaped by the interactions with the wind of the host star. The stellar wind is formed by particles and magnetic fields that shape the exo-spac
Externí odkaz:
http://arxiv.org/abs/2309.00324
Publikováno v:
Frontiers in Oncology, Vol 8 (2018)
Externí odkaz:
https://doaj.org/article/23662a0ecaaf4bcea43f31259a59df2b
Autor:
Nowacki, H., Alecian, E., Perraut, K., Zaire, B., Folsom, C. P., Pouilly, K., Bouvier, J., Manick, R., Pantolmos, G., Sousa, A. P., Dougados, C., Hussain, G. A. J., Alencar, S. H. P., Bouquin, J. B. Le
Publikováno v:
A&A 678, A86 (2023)
Aims : We aimed at constraining the accretion-ejection phenomena around the strongly-accreting Northern component of the S CrA young binary system (S CrA N) by deriving its magnetic field topology and its magnetospheric properties, and by detecting e
Externí odkaz:
http://arxiv.org/abs/2308.03442