Zobrazeno 1 - 10
of 2 273
pro vyhledávání: '"Egorova E"'
Autor:
Chudakova, T. A., Mazhorin, G. S., Trofimov, I. V., Rudenko, N. Yu., Mumlyakov, A. M., Kazmina, A. S., Egorova, E. Yu., Gladilovich, P. A., Chichkov, M. V., Maleeva, N. A., Tarkhov, M. A., Chichkov, V. I.
Publikováno v:
JETP Letters, Vol. 120, No. 4, pp. 298-305, 2024
Superconducting qubits are considered as a promising platform for implementing a fault tolerant quantum computing. However, surface defects of superconductors and the substrate leading to qubit state decoherence and fluctuations in qubit parameters c
Externí odkaz:
http://arxiv.org/abs/2409.16097
Autor:
Kreckel, K., Egorov, O. V., Egorova, E., Blanc, G. A., Drory, N., Kounkel, M., Mendez-Delgado, J. E., Roman-Zuniga, C. G., Sanchez, S. F., Stringfellow, G. S., Stutz, A. M., Zari, E., Barrera-Ballesteros, J. K., Bizyaev, D., Brownstein, J. R., Congiu, E., Fernandez-Trincado, J. G., Garcia, P., Hillenbrand, L., Ibarra-Medel, H. J., Jin, Y., Johnston, E. J., Jones, A. M., Kim, J. Serena, Kollmeier, J. A., Kong, S., Krishnarao, D., Kumari, N., Li, J., Long, K., Mata-Sanchez, A., Mejia-Narvaez, A., Popa, S. A., Rix, H-W, Sattler, N., Serna, J., Singh, A., Sanchez-Gallego, J. R., Wofford, A., Wong, T.
Publikováno v:
A&A 689, A352 (2024)
The Orion Molecular Cloud complex, one of the nearest (D = 406 pc) and most extensively studied massive star-forming regions, is ideal for constraining the physics of stellar feedback, but its ~12 deg diameter on the sky requires a dedicated approach
Externí odkaz:
http://arxiv.org/abs/2405.14943
In the framework of the ongoing project, aimed at the systematical studying galaxies in nearby voids, we conducted spectroscopy with the Southern African Large Telescope (SALT) of 62 objects from the Nearby Void Galaxy (NVG) sample. They include 8 re
Externí odkaz:
http://arxiv.org/abs/2312.07815
Autor:
Pustilnik, S., Perepelitsyna, Y., Tepliakova, A., Kniazev, A., Egorova, E., Chengalur, J., Kurapati, S.
Voids occupy about 3/4 of the volume of the Universe and contain about 15% of its mass. Due to various observational selection effects, these structure elements and galaxies populating voids, are highly under-explored. This especially relates to the
Externí odkaz:
http://arxiv.org/abs/2212.05640
Autor:
Pustilnik, S. A., Egorova, E. S., Kniazev, A. Y., Perepelitsyna, Y. A., Tepliakova, A. L., Burenkov, A. N., Oparin, D. V.
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 507, Issue 1, October 2021, Pages 944-962
We present the second part of results of the on-going project of searching for and studying eXtremely Metal-Poor (XMP, adopted as those with Z(gas) <~ Zo/30, or with 12+log(O/H) <~ 7.21~dex) very gas-rich blue dwarfs in voids.They were first identifi
Externí odkaz:
http://arxiv.org/abs/2108.12065
Autor:
Egorova, E. S., Egorov, O. V., Moiseev, A. V., Saburova, A. S., Grishin, K. A., Chilingarian, I. V.
The low-mass low-surface brightness (LSB) disc galaxy Arakelian 18 (Ark 18) resides in the Eridanus void and because of its isolation represents an ideal case to study the formation and evolution mechanisms of such a galaxy type. Its complex structur
Externí odkaz:
http://arxiv.org/abs/2103.00211
Autor:
Fedorov, G. P., Remizov, S. V., Shapiro, D. S., Pogosov, W. V., Egorova, E., Tsitsilin, I., Andronik, M., Dobronosova, A. A., Rodionov, I. A., Astafiev, O. V., Ustinov, A. V.
Publikováno v:
Phys. Rev. Lett. 126, 180503 (2021)
We demonstrate non-equilibrium steady-state photon transport through a chain of five coupled artificial atoms simulating the driven-dissipative Bose-Hubbard model. Using transmission spectroscopy, we show that the system retains many-particle coheren
Externí odkaz:
http://arxiv.org/abs/2011.11454
In the framework of an ongoing project aimed at searching for and studying eXtremely Metal-Poor (XMP) very gas-rich blue dwarfs in nearby voids, we conducted spectroscopy with the 11-m Southern African Large Telescope (SALT) of 26 candidates, presele
Externí odkaz:
http://arxiv.org/abs/1912.06857
We introduce a project aimed at systematically searching for eXtremely Metal-Poor (XMP) very gas-rich blue dwarfs in voids in the nearby Universe. Several such galaxies were first identified in the course of an unbiased study of the galaxy population
Externí odkaz:
http://arxiv.org/abs/1912.06740
Half-dozen of extreme representatives of void dwarf galaxy population were found in our study of evolutionary status of a hundred galaxies in the nearby Lynx-Cancer void. They are very gas-rich, extremely low-metallicity [7.0 < 12+log(O/H)< ~7.3] obj
Externí odkaz:
http://arxiv.org/abs/1812.04473