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A KINEMATIC STUDY OF THE INTERACTING-SYSTEM NGC-5953/54. / RESHETNIKOV, VP.

In: АСТРОНОМИЧЕСКИЙ ЖУРНАЛ, Vol. 70, No. 1, 1993, p. 216-220.

Research output: Contribution to journal › Comment/debate › peer-review

Harvard

RESHETNIKOV, VP 1993, 'A KINEMATIC STUDY OF THE INTERACTING-SYSTEM NGC-5953/54', АСТРОНОМИЧЕСКИЙ ЖУРНАЛ, vol. 70, no. 1, pp. 216-220.

APA

RESHETNIKOV, VP. (1993). A KINEMATIC STUDY OF THE INTERACTING-SYSTEM NGC-5953/54. АСТРОНОМИЧЕСКИЙ ЖУРНАЛ, 70(1), 216-220.

Vancouver

RESHETNIKOV VP. A KINEMATIC STUDY OF THE INTERACTING-SYSTEM NGC-5953/54. АСТРОНОМИЧЕСКИЙ ЖУРНАЛ. 1993;70(1):216-220.

Author

RESHETNIKOV, VP. / A KINEMATIC STUDY OF THE INTERACTING-SYSTEM NGC-5953/54. In: АСТРОНОМИЧЕСКИЙ ЖУРНАЛ. 1993 ; Vol. 70, No. 1. pp. 216-220.

BibTeX

@article{3ef9b847426b48888f0ef9b1c1770d5e,
title = "A KINEMATIC STUDY OF THE INTERACTING-SYSTEM NGC-5953/54",
abstract = "The results of the detailed kinematic study of the pair of interacing galaxies NGC 5953/54 (Arp 91, VV 244, Mrk 1512) are presented. The spectral observations of the members of the pair were made using 2,6-m telescope of Buyrakan Astrophysical Observatory and 6-m telescope of Special Astrophysical Observatory. The heliocentric systemic velocities of the galaxies are 1994+/-5 km/s (NGC 5953) and 1848+/-10 km/s (NGC 5954). The derived rotation curves of galaxies show a significant asymmetry and at different position angles demonstate both decrease and increase of radial velocities as compared with circular motion. The standard kinematical parameters of galaxies a.re determined.",
author = "VP RESHETNIKOV",
year = "1993",
language = "не определен",
volume = "70",
pages = "216--220",
journal = "АСТРОНОМИЧЕСКИЙ ЖУРНАЛ",
issn = "0004-6299",
publisher = "Международная книга",
number = "1",

}

RIS

TY - JOUR

T1 - A KINEMATIC STUDY OF THE INTERACTING-SYSTEM NGC-5953/54

AU - RESHETNIKOV, VP

PY - 1993

Y1 - 1993

N2 - The results of the detailed kinematic study of the pair of interacing galaxies NGC 5953/54 (Arp 91, VV 244, Mrk 1512) are presented. The spectral observations of the members of the pair were made using 2,6-m telescope of Buyrakan Astrophysical Observatory and 6-m telescope of Special Astrophysical Observatory. The heliocentric systemic velocities of the galaxies are 1994+/-5 km/s (NGC 5953) and 1848+/-10 km/s (NGC 5954). The derived rotation curves of galaxies show a significant asymmetry and at different position angles demonstate both decrease and increase of radial velocities as compared with circular motion. The standard kinematical parameters of galaxies a.re determined.

AB - The results of the detailed kinematic study of the pair of interacing galaxies NGC 5953/54 (Arp 91, VV 244, Mrk 1512) are presented. The spectral observations of the members of the pair were made using 2,6-m telescope of Buyrakan Astrophysical Observatory and 6-m telescope of Special Astrophysical Observatory. The heliocentric systemic velocities of the galaxies are 1994+/-5 km/s (NGC 5953) and 1848+/-10 km/s (NGC 5954). The derived rotation curves of galaxies show a significant asymmetry and at different position angles demonstate both decrease and increase of radial velocities as compared with circular motion. The standard kinematical parameters of galaxies a.re determined.

M3 - комментарий, выступление

VL - 70

SP - 216

EP - 220

JO - АСТРОНОМИЧЕСКИЙ ЖУРНАЛ

JF - АСТРОНОМИЧЕСКИЙ ЖУРНАЛ

SN - 0004-6299

IS - 1

ER -

ID: 32476710