Zobrazeno 1 - 10
of 117
pro vyhledávání: '"Zaitseva, Natalia P."'
Publikováno v:
St. Petersburg State Polytechnical University Journal. Physics and Mathematics, 2023, v.16 (1.2), pp.395-402
Recent studies show the possibility of the formation of fairly regular and global spiral patterns in dwarf galaxies (dS type). Our sample of observed dwarf objects of this class also includes galaxies with a central stellar bar. The analysis of the o
Externí odkaz:
http://arxiv.org/abs/2307.15925
Autor:
Ford, Michael J., Aigeldinger, Elisabeth, Sutanto, Felicia, Zaitseva, Natalia P., Li, Viacheslav A., Carman, M. Leslie, Glenn, Andrew, Catala, Cristian R., Dazeley, Steven A., Bowden, Nathaniel
Plastic scintillators that can discriminate between gamma rays, fast neutrons, and thermal neutrons were synthesized and characterized while considering the balance between processing and performance at the kilogram scale. These trade-offs were neces
Externí odkaz:
http://arxiv.org/abs/2301.04185
Publikováno v:
Astronomy Reports, Vol. 66, No. 9, pp. 755-765, 2022
The content of gas in galaxies with an anomalously high relative mass of hydrogen $M_{HI}/M_*$ for a given mass of the stellar population $M_*$ (VHR-galaxies) is considered, using the available samples of such galaxies. It is shown that, within the o
Externí odkaz:
http://arxiv.org/abs/2211.14001
Autor:
Ford, Michael J., Zaitseva, Natalia P., Carman, M. Leslie, Dazeley, Steven A., Bernstein, Adam, Glenn, Andrew, Akindele, Oluwatomi A.
This work describes a class of liquid scintillators that contain mostly water (>50 wt. % of the entire composition) and can discriminate between interactions induced by neutrons and gamma rays. By balancing the interface interactions between the comp
Externí odkaz:
http://arxiv.org/abs/2202.07625
Spiral structure (both flocculent and Grand Design types) is very rarely observed in dwarf galaxies because the formation of spiral arms requires special conditions. In this work we analyze the sample of about 40 dS-galaxies found by scanning by eye
Externí odkaz:
http://arxiv.org/abs/2108.04624
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We examine the dependence between hydrogen total mass $M_{HI}$ and rotation speed $V_{rot}$, optical size $D_{25}$ or disc radial scale $R_0$ for two samples of late-type galaxies: a) isolated galaxy (AMIGA sample), and b) the edge-on galaxies (flat
Externí odkaz:
http://arxiv.org/abs/1705.07659
Autor:
Lance, Michael J., Zaitseva, Natalia P., Payne, Stephen A., Kouzes, Richard T., Myllenbeck, Nicholas R., Janos, Alan
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A 21 February 2020 954
Autor:
Langeveld, Willem G.J., Glenn, Andrew M., Sheets, Steven A., Strellis, Dan A., Zaitseva, Natalia P.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A 21 February 2020 954
Akademický článek
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