Standard

ON THE ROTATIONAL VELOCITIES OF INTERACTING GALAXIES. / RESHETNIKOV, VP.

в: Astrophysics and Space Science, Том 211, № 1, 01.1994, стр. 155-160.

Результаты исследований: Научные публикации в периодических изданиях › письмо/краткое сообщение › Рецензирование

Harvard

RESHETNIKOV, VP 1994, 'ON THE ROTATIONAL VELOCITIES OF INTERACTING GALAXIES', Astrophysics and Space Science, Том. 211, № 1, стр. 155-160. https://doi.org/10.1007/BF00658049, https://doi.org/10.1007/BF00658049

APA

RESHETNIKOV, VP. (1994). ON THE ROTATIONAL VELOCITIES OF INTERACTING GALAXIES. Astrophysics and Space Science, 211(1), 155-160. https://doi.org/10.1007/BF00658049, https://doi.org/10.1007/BF00658049

Vancouver

RESHETNIKOV VP. ON THE ROTATIONAL VELOCITIES OF INTERACTING GALAXIES. Astrophysics and Space Science. 1994 Янв.;211(1):155-160. https://doi.org/10.1007/BF00658049, https://doi.org/10.1007/BF00658049

Author

RESHETNIKOV, VP. / ON THE ROTATIONAL VELOCITIES OF INTERACTING GALAXIES. в: Astrophysics and Space Science. 1994 ; Том 211, № 1. стр. 155-160.

BibTeX

@article{2d5628d417964ae8a8ae91de821eabc9,
title = "ON THE ROTATIONAL VELOCITIES OF INTERACTING GALAXIES",
abstract = "A sample of members of close-binary interacting galaxies with the known values of the maximum rotational velocities are considered. It is found that the spiral galaxies in interacting systems tend to have lower rotational velocities and smaller mass to luminosity ratios than their counterparts in the field. The Tully-Fisher relationship may be different for interacting and field galaxies.",
keywords = "PAIR",
author = "VP RESHETNIKOV",
year = "1994",
month = jan,
doi = "10.1007/BF00658049",
language = "Английский",
volume = "211",
pages = "155--160",
journal = "Astrophysics and Space Science",
issn = "0004-640X",
publisher = "Wolters Kluwer",
number = "1",

}

RIS

TY - JOUR

T1 - ON THE ROTATIONAL VELOCITIES OF INTERACTING GALAXIES

AU - RESHETNIKOV, VP

PY - 1994/1

Y1 - 1994/1

N2 - A sample of members of close-binary interacting galaxies with the known values of the maximum rotational velocities are considered. It is found that the spiral galaxies in interacting systems tend to have lower rotational velocities and smaller mass to luminosity ratios than their counterparts in the field. The Tully-Fisher relationship may be different for interacting and field galaxies.

AB - A sample of members of close-binary interacting galaxies with the known values of the maximum rotational velocities are considered. It is found that the spiral galaxies in interacting systems tend to have lower rotational velocities and smaller mass to luminosity ratios than their counterparts in the field. The Tully-Fisher relationship may be different for interacting and field galaxies.

KW - PAIR

U2 - 10.1007/BF00658049

DO - 10.1007/BF00658049

M3 - письмо/краткое сообщение

VL - 211

SP - 155

EP - 160

JO - Astrophysics and Space Science

JF - Astrophysics and Space Science

SN - 0004-640X

IS - 1

ER -

ID: 32476260