Zobrazeno 1 - 10
of 435
pro vyhledávání: '"M. M. Romanova"'
Publikováno v:
The Sixteenth Marcel Grossmann Meeting.
Autor:
Catherine Espaillat, C. E. Robinson, Mark Reynolds, Thanawuth Thanathibodee, Nuria Calvet, M. M. Romanova, J. Wendeborn, James Muzerolle
Publikováno v:
Nature
Magnetospheric accretion models predict that matter from protoplanetary disks accretes onto the star via funnel flows which follow the stellar field lines and shock on the stellar surface leaving a hot spot with a density gradient. Previous work has
Publikováno v:
The Fifteenth Marcel Grossmann Meeting.
Autor:
M. M. Romanova, A. P. Babkin
Publikováno v:
Российский кардиологический журнал, Vol 0, Iss 4, Pp 30-36 (2012)
Aim. To study psycho-emotional and autonomic status, circadian blood pressure (BP) profile, and quality of life (QoL) in patients with metabolic syndrome (MS) and dyspepsia syndrome. Material and methods. We followed up 110 patients (66 women and 52
Externí odkaz:
https://doaj.org/article/a2cf4ec5b1e4455995d6192d34017b81
Autor:
M. M. Romanova, T. E. Galdina
Publikováno v:
Polythematic Online Scientific Journal of Kuban State Agrarian University.
Publikováno v:
Klinicheskaia meditsina. 91(9)
Disordered eating behavior, nutritional regime, and food habits lead to deterioration of quality of life especially in patients with digestive problems. The role of nutrition in etiology and pathogenesis of dyspepsia is currently the subject of incre
Publikováno v:
Voprosy pitaniia. 82(1)
Recent years, restructuring of the health care to the population, including a complex of measures to improve the human resources policy in health, spurring the practice of the disciplines to public health care, turning, organizing 3-tier health care
Autor:
R. V. E. Lovelace, M. M. Romanova, G. V. Ustyugova, A. V. Koldoba, Giuseppe Bertin, Franca De Luca, Giuseppe Lodato, Roberto Pozzoli, Massimiliano Romé
Publikováno v:
AIP Conference Proceedings.
We investigate the launching of outflows from the disk‐magnetosphere boundary of slowly and rapidly rotating magnetized stars using axisymmetric magnetohydrodynamic (MHD) simulations. We find long‐lasting outflows in both cases. (1) In the case o
Autor:
M. M. Romanova, A. K. Kulkarni, M. Long, R. V. E. Lovelace, Rudy Wijnands, Diego Altamirano, Paolo Soleri, Nathalie Degenaar, Nanda Rea, Piergiorgio Casella, Alessandro Patruno, Manuel Linares
The appearance and time variability of accreting millisecond X-ray pulsars (hereafter AMXPs, e.g. Wijnands & van der Klis 1998) depends strongly on the accretion rate, the effective viscosity and the effective magnetic diffusivity of the disk-magneto
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8b9302d96041a38d2905a172deb4c073
http://arxiv.org/abs/0812.2890
http://arxiv.org/abs/0812.2890
Autor:
A. K. Kulkarni, M. M. Romanova, Rudy Wijnands, Diego Altamirano, Paolo Soleri, Nathalie Degenaar, Nanda Rea, Piergiorgio Casella, Alessandro Patruno, Manuel Linares
We present results of 3D simulations of MHD instabilities at the accretion disk-magnetosphere boundary. The instability is Rayleigh-Taylor, and develops for a fairly broad range of accretion rates and stellar rotation rates and magnetic fields. It pr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::40b756e1cd5598c671d7f76e73ae2a9f
http://arxiv.org/abs/0812.2239
http://arxiv.org/abs/0812.2239