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UGC 7388 : A galaxy with two tidal loops. / Faúndez-Abans, M.; Reshetnikov, V. P.; De Oliveira-Abans, M.; Fernandes, I. F.

в: Astronomy Letters, Том 35, № 1, 01.01.2009, стр. 25-32.

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

Harvard

Faúndez-Abans, M, Reshetnikov, VP, De Oliveira-Abans, M & Fernandes, IF 2009, 'UGC 7388: A galaxy with two tidal loops', Astronomy Letters, Том. 35, № 1, стр. 25-32. https://doi.org/10.1134/S1063773709010034

APA

Faúndez-Abans, M., Reshetnikov, V. P., De Oliveira-Abans, M., & Fernandes, I. F. (2009). UGC 7388: A galaxy with two tidal loops. Astronomy Letters, 35(1), 25-32. https://doi.org/10.1134/S1063773709010034

Vancouver

Faúndez-Abans M, Reshetnikov VP, De Oliveira-Abans M, Fernandes IF. UGC 7388: A galaxy with two tidal loops. Astronomy Letters. 2009 Янв. 1;35(1):25-32. https://doi.org/10.1134/S1063773709010034

Author

Faúndez-Abans, M. ; Reshetnikov, V. P. ; De Oliveira-Abans, M. ; Fernandes, I. F. / UGC 7388 : A galaxy with two tidal loops. в: Astronomy Letters. 2009 ; Том 35, № 1. стр. 25-32.

BibTeX

@article{f5ae081c8bae474baab921cb9c908fde,
title = "UGC 7388: A galaxy with two tidal loops",
abstract = "We present the results of our spectroscopic and morphological studies of the galaxy UGC 7388 with the 8.1-m Gemini North telescope. Judging by its observed characteristics, UGC 7388 is a giant late-type spiral galaxy seen nearly edge-on. The main body of the galaxy is surrounded by two faint (μ B ∼ 24 m ∼ and μ B ∼ 25 • m 5/∼) extended (∼ 20-30 kpc) loop-like structures. A large-scale rotation of the brighter loop about the main galaxy has been detected. We discuss the assumption that the tidal disruption of a relatively massive companion is observed in the case of UGC 7388. A detailed study and modeling of the observed structure of this unique galaxy can give important information about the influence of the absorption of massive companions on the galactic disks and about the structure of the dark halo around UGC 7388.",
keywords = "Galaxies, Interacting galaxies, Kinematics, Morphology",
author = "M. Fa{\'u}ndez-Abans and Reshetnikov, {V. P.} and {De Oliveira-Abans}, M. and Fernandes, {I. F.}",
year = "2009",
month = jan,
day = "1",
doi = "10.1134/S1063773709010034",
language = "English",
volume = "35",
pages = "25--32",
journal = "Astronomy Letters",
issn = "1063-7737",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "1",

}

RIS

TY - JOUR

T1 - UGC 7388

T2 - A galaxy with two tidal loops

AU - Faúndez-Abans, M.

AU - Reshetnikov, V. P.

AU - De Oliveira-Abans, M.

AU - Fernandes, I. F.

PY - 2009/1/1

Y1 - 2009/1/1

N2 - We present the results of our spectroscopic and morphological studies of the galaxy UGC 7388 with the 8.1-m Gemini North telescope. Judging by its observed characteristics, UGC 7388 is a giant late-type spiral galaxy seen nearly edge-on. The main body of the galaxy is surrounded by two faint (μ B ∼ 24 m ∼ and μ B ∼ 25 • m 5/∼) extended (∼ 20-30 kpc) loop-like structures. A large-scale rotation of the brighter loop about the main galaxy has been detected. We discuss the assumption that the tidal disruption of a relatively massive companion is observed in the case of UGC 7388. A detailed study and modeling of the observed structure of this unique galaxy can give important information about the influence of the absorption of massive companions on the galactic disks and about the structure of the dark halo around UGC 7388.

AB - We present the results of our spectroscopic and morphological studies of the galaxy UGC 7388 with the 8.1-m Gemini North telescope. Judging by its observed characteristics, UGC 7388 is a giant late-type spiral galaxy seen nearly edge-on. The main body of the galaxy is surrounded by two faint (μ B ∼ 24 m ∼ and μ B ∼ 25 • m 5/∼) extended (∼ 20-30 kpc) loop-like structures. A large-scale rotation of the brighter loop about the main galaxy has been detected. We discuss the assumption that the tidal disruption of a relatively massive companion is observed in the case of UGC 7388. A detailed study and modeling of the observed structure of this unique galaxy can give important information about the influence of the absorption of massive companions on the galactic disks and about the structure of the dark halo around UGC 7388.

KW - Galaxies

KW - Interacting galaxies

KW - Kinematics

KW - Morphology

UR - http://www.scopus.com/inward/record.url?scp=58149520257&partnerID=8YFLogxK

U2 - 10.1134/S1063773709010034

DO - 10.1134/S1063773709010034

M3 - Article

AN - SCOPUS:58149520257

VL - 35

SP - 25

EP - 32

JO - Astronomy Letters

JF - Astronomy Letters

SN - 1063-7737

IS - 1

ER -

ID: 36180785