Zobrazeno 1 - 10
of 13
pro vyhledávání: '"I. A. Acharova"'
Publikováno v:
Odessa Astronomical Publications, Vol 21, Iss 0, Pp 9-12 (2008)
The goal of paper to see that different models for spiral pattern of galactic disks lead to distinguishable radial distribution of heavy elements. Moreover it will be explained why the distributions, demonstrated different chemical elements show diff
Externí odkaz:
https://doaj.org/article/d1ff15dd1fb6461a873349107571e129
A method is proposed for determining the properties of type Ia supernovae from short-lived precursors -- Prompt SNIa. This method is based on the assumption that this subtype of type Ia supernovae exploded into low-metallicity globular clusters (GCs)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::98c4726bda5e988d8d8e1f486a1e7b4b
On the relationship between metallicity distributions of globular clusters and of circumgalactic gas
Autor:
Margarita Sharina, I. A. Acharova
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 481:2074-2082
The abundance of alpha elements and iron in stars of globular clusters shows the composition of the gaseous medium, in which they have been formed. In the present paper, we discuss a possibility to consider dense clouds of circumgalactic gas (partial
Autor:
E. S. Shevtsova, I. A. Acharova
Publikováno v:
Astrophysical Bulletin. 71:24-32
We discuss the possibility of finding the birthplaces of open clusters (OC) with ages of several billion years. The proposed method is based on the comparison of the results of the chemical evolution modeling of the Galactic disk with the parameters
Autor:
M. E. Sharina, I. A. Acharova
Publikováno v:
Астрономия-2018. Том 1.
Publikováno v:
Astrophysical Bulletin. 69:21-26
A new mechanism of sweeping out of dust grains beyond galactic disks both in the radial direction along the galactic plane and in the vertical, cross-disk direction is proposed. The mechanism is driven by the interaction of dust grains with the bisym
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 420:1590-1605
We propose a statistical method for decomposition of contributions to iron production from various sources: Type II supernovae and the subpopulations of Type Ia supernovae, prompt (their progenitors are short-lived stars with ages lower than ∼100 M
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 415:L11-L15
We propose a new method for determination of the rotation velocity of the galactic spiral density waves, correspondingly, the corotation radius, $r_C$, in our Galaxy by means of statistical analysis of radial oxygen distribution in the galactic disc
Autor:
Yu. N. Mishurov, I. A. Acharova
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 412:1771-1777
We present the results of our numerical experiments on stellar scattering in the Galactic disc under the influence of the perturbed Galactic gravitational field associated with spiral density waves. We show that the view according to which stars do n
Autor:
Yu. N. Mishurov, I. A. Acharova, A. V. Tutukov, Jacques Raymond Daniel Lépine, Dmitri Wiebe, Boris Shustov
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 402:1149-1155
Recently, it has been proposed that there are two type Ia supernova progenitors: short-lived and long-lived. On the basis of this idea, we develop a theory of a unified mechanism for the formation of the bimodal radial distribution of iron and oxygen