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Rotation curves of galaxies in various space environments. / Evstigneeva, E. A.; Reshetnikov, V. P.

в: Astrophysics, Том 44, № 2, 01.01.2001, стр. 158-162.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Evstigneeva, EA & Reshetnikov, VP 2001, 'Rotation curves of galaxies in various space environments', Astrophysics, Том. 44, № 2, стр. 158-162. https://doi.org/10.1023/A:1010932406542

APA

Evstigneeva, E. A., & Reshetnikov, V. P. (2001). Rotation curves of galaxies in various space environments. Astrophysics, 44(2), 158-162. https://doi.org/10.1023/A:1010932406542

Vancouver

Evstigneeva EA, Reshetnikov VP. Rotation curves of galaxies in various space environments. Astrophysics. 2001 Янв. 1;44(2):158-162. https://doi.org/10.1023/A:1010932406542

Author

Evstigneeva, E. A. ; Reshetnikov, V. P. / Rotation curves of galaxies in various space environments. в: Astrophysics. 2001 ; Том 44, № 2. стр. 158-162.

BibTeX

@article{cee1fb0b5e6b47b090481d4f1b31aabc,
title = "Rotation curves of galaxies in various space environments",
abstract = "A sample of giant Sb-Sc spiral galaxies for which there are highly accurate and extended rotation curves was considered. Having divided the galaxies into three groups as a function of the overall spatial density of luminosity (mass) within 0.5 Mpc (ρL), we investigated the characteristics of the rotation curves as functions of ρL. It turned out that for such massive galaxies, the shape of the rotation curve (the logarithmic gradient) and the Tully-Fisher relation do not depend on the overall space environment. The only difference is that the rotation curves of galaxies in regions with high ρL can be traced out to smaller relative distances from the nucleus, on the average. This may be related to destruction of the outer regions of their gaseous disks in gravitational interaction with surrounding galaxies.",
author = "Evstigneeva, {E. A.} and Reshetnikov, {V. P.}",
year = "2001",
month = jan,
day = "1",
doi = "10.1023/A:1010932406542",
language = "English",
volume = "44",
pages = "158--162",
journal = "Astrophysics",
issn = "0571-7256",
publisher = "Wolters Kluwer",
number = "2",

}

RIS

TY - JOUR

T1 - Rotation curves of galaxies in various space environments

AU - Evstigneeva, E. A.

AU - Reshetnikov, V. P.

PY - 2001/1/1

Y1 - 2001/1/1

N2 - A sample of giant Sb-Sc spiral galaxies for which there are highly accurate and extended rotation curves was considered. Having divided the galaxies into three groups as a function of the overall spatial density of luminosity (mass) within 0.5 Mpc (ρL), we investigated the characteristics of the rotation curves as functions of ρL. It turned out that for such massive galaxies, the shape of the rotation curve (the logarithmic gradient) and the Tully-Fisher relation do not depend on the overall space environment. The only difference is that the rotation curves of galaxies in regions with high ρL can be traced out to smaller relative distances from the nucleus, on the average. This may be related to destruction of the outer regions of their gaseous disks in gravitational interaction with surrounding galaxies.

AB - A sample of giant Sb-Sc spiral galaxies for which there are highly accurate and extended rotation curves was considered. Having divided the galaxies into three groups as a function of the overall spatial density of luminosity (mass) within 0.5 Mpc (ρL), we investigated the characteristics of the rotation curves as functions of ρL. It turned out that for such massive galaxies, the shape of the rotation curve (the logarithmic gradient) and the Tully-Fisher relation do not depend on the overall space environment. The only difference is that the rotation curves of galaxies in regions with high ρL can be traced out to smaller relative distances from the nucleus, on the average. This may be related to destruction of the outer regions of their gaseous disks in gravitational interaction with surrounding galaxies.

UR - http://www.scopus.com/inward/record.url?scp=52549092190&partnerID=8YFLogxK

U2 - 10.1023/A:1010932406542

DO - 10.1023/A:1010932406542

M3 - Article

AN - SCOPUS:52549092190

VL - 44

SP - 158

EP - 162

JO - Astrophysics

JF - Astrophysics

SN - 0571-7256

IS - 2

ER -

ID: 36180180