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A spectroscopic study of the peculiar galaxy UGC 5600. / Shalyapina, L. V.; Moiseev, A. V.; Yakovleva, V. A.

в: Astronomy Letters, Том 28, № 7, 07.2002, стр. 443-453.

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

Harvard

Shalyapina, LV, Moiseev, AV & Yakovleva, VA 2002, 'A spectroscopic study of the peculiar galaxy UGC 5600', Astronomy Letters, Том. 28, № 7, стр. 443-453. https://doi.org/10.1134/1.1491967

APA

Shalyapina, L. V., Moiseev, A. V., & Yakovleva, V. A. (2002). A spectroscopic study of the peculiar galaxy UGC 5600. Astronomy Letters, 28(7), 443-453. https://doi.org/10.1134/1.1491967

Vancouver

Shalyapina LV, Moiseev AV, Yakovleva VA. A spectroscopic study of the peculiar galaxy UGC 5600. Astronomy Letters. 2002 Июль;28(7):443-453. https://doi.org/10.1134/1.1491967

Author

Shalyapina, L. V. ; Moiseev, A. V. ; Yakovleva, V. A. / A spectroscopic study of the peculiar galaxy UGC 5600. в: Astronomy Letters. 2002 ; Том 28, № 7. стр. 443-453.

BibTeX

@article{f15e2487105b4378822a782f3873bf71,
title = "A spectroscopic study of the peculiar galaxy UGC 5600",
abstract = "We present our observations of the galaxy UGS 5600 with a long-slit spectrograph (UAGS) and a multipupil field spectrograph (MPFS) attached to the 6-m Special Astrophysical Observatory telescope. Radial-velocity fields of the stellar and gaseous components were constructed for the central region and inner ring of the galaxy. We proved the existence of two nearly orthogonal kinematic subsystems and conclude that UGC 5600 is a galaxy with an inner polar ring. In the circumnuclear region, we detected noncircular stellar motions and suspected the existence of a minibar. The emission lines are shown to originate in H II regions. We estimated the metalliciiy from the intensity ratio of the [N II]λ6583 and Hα lines to be nearly solar, which rules out the possibility that the polar ring was produced by the accretion of gas from a dwarf companion.",
keywords = "Kinematics, Polar-ring galaxies, UGC 5600",
author = "Shalyapina, {L. V.} and Moiseev, {A. V.} and Yakovleva, {V. A.}",
year = "2002",
month = jul,
doi = "10.1134/1.1491967",
language = "English",
volume = "28",
pages = "443--453",
journal = "Astronomy Letters",
issn = "1063-7737",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "7",

}

RIS

TY - JOUR

T1 - A spectroscopic study of the peculiar galaxy UGC 5600

AU - Shalyapina, L. V.

AU - Moiseev, A. V.

AU - Yakovleva, V. A.

PY - 2002/7

Y1 - 2002/7

N2 - We present our observations of the galaxy UGS 5600 with a long-slit spectrograph (UAGS) and a multipupil field spectrograph (MPFS) attached to the 6-m Special Astrophysical Observatory telescope. Radial-velocity fields of the stellar and gaseous components were constructed for the central region and inner ring of the galaxy. We proved the existence of two nearly orthogonal kinematic subsystems and conclude that UGC 5600 is a galaxy with an inner polar ring. In the circumnuclear region, we detected noncircular stellar motions and suspected the existence of a minibar. The emission lines are shown to originate in H II regions. We estimated the metalliciiy from the intensity ratio of the [N II]λ6583 and Hα lines to be nearly solar, which rules out the possibility that the polar ring was produced by the accretion of gas from a dwarf companion.

AB - We present our observations of the galaxy UGS 5600 with a long-slit spectrograph (UAGS) and a multipupil field spectrograph (MPFS) attached to the 6-m Special Astrophysical Observatory telescope. Radial-velocity fields of the stellar and gaseous components were constructed for the central region and inner ring of the galaxy. We proved the existence of two nearly orthogonal kinematic subsystems and conclude that UGC 5600 is a galaxy with an inner polar ring. In the circumnuclear region, we detected noncircular stellar motions and suspected the existence of a minibar. The emission lines are shown to originate in H II regions. We estimated the metalliciiy from the intensity ratio of the [N II]λ6583 and Hα lines to be nearly solar, which rules out the possibility that the polar ring was produced by the accretion of gas from a dwarf companion.

KW - Kinematics

KW - Polar-ring galaxies

KW - UGC 5600

UR - http://www.scopus.com/inward/record.url?scp=0036638505&partnerID=8YFLogxK

U2 - 10.1134/1.1491967

DO - 10.1134/1.1491967

M3 - Article

AN - SCOPUS:0036638505

VL - 28

SP - 443

EP - 453

JO - Astronomy Letters

JF - Astronomy Letters

SN - 1063-7737

IS - 7

ER -

ID: 52305194