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Photometric structure of polar-ring galaxies. / Reshetnikov, VP.

In: ASTRONOMY & ASTROPHYSICS, Vol. 416, No. 3, 03.2004, p. 889-900.

Research output: Contribution to journal › Article › peer-review

Harvard

Reshetnikov, VP 2004, 'Photometric structure of polar-ring galaxies', ASTRONOMY & ASTROPHYSICS, vol. 416, no. 3, pp. 889-900. https://doi.org/10.1051/0004-6361:20031382

APA

Reshetnikov, VP. (2004). Photometric structure of polar-ring galaxies. ASTRONOMY & ASTROPHYSICS, 416(3), 889-900. https://doi.org/10.1051/0004-6361:20031382

Vancouver

Reshetnikov VP. Photometric structure of polar-ring galaxies. ASTRONOMY & ASTROPHYSICS. 2004 Mar;416(3):889-900. https://doi.org/10.1051/0004-6361:20031382

Author

Reshetnikov, VP. / Photometric structure of polar-ring galaxies. In: ASTRONOMY & ASTROPHYSICS. 2004 ; Vol. 416, No. 3. pp. 889-900.

BibTeX

@article{3308a71317ad48f4aadab7813de47124,
title = "Photometric structure of polar-ring galaxies",
abstract = "The results of B, V, R surface photometry of three polar-ring galaxies (PRGs) - A 0017+2212, UGC 1198, UGC 4385 - are presented. The data were acquired at the 6-m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences. It was shown that all three galaxies are peculiar late-type spirals in the state of ongoing interaction or merging.We discuss available photometric properties of the PRGs with spiral hosts and consider the Tully-Fisher relation for different types of PRGs. In agreement with Iodice et al. (2003), we have shown that true PRGs demonstrate similar to1/3 larger maximum rotation velocities than spiral galaxies of the same luminosity. Peculiar objects with forming polar structures satisfy, on average, the Tully-Fisher relation for disk galaxies but with large scatter.",
keywords = "galaxies : individual : A 0017+2212, UGC 1198, UGC 4385, galaxies : photometry, galaxies : formation, galaxies : structure, NEAR-INFRARED PHOTOMETRY, TULLY-FISHER RELATION, INTERACTING GALAXIES, IRAS OBSERVATIONS, GLOBAL STRUCTURE, SPIRAL GALAXIES, DARK HALO, KN-BANDS, H-BANDS, DISK",
author = "VP Reshetnikov",
year = "2004",
month = mar,
doi = "10.1051/0004-6361:20031382",
language = "Английский",
volume = "416",
pages = "889--900",
journal = "ASTRONOMY & ASTROPHYSICS",
issn = "0004-6361",
publisher = "EDP Sciences",
number = "3",

}

RIS

TY - JOUR

T1 - Photometric structure of polar-ring galaxies

AU - Reshetnikov, VP

PY - 2004/3

Y1 - 2004/3

N2 - The results of B, V, R surface photometry of three polar-ring galaxies (PRGs) - A 0017+2212, UGC 1198, UGC 4385 - are presented. The data were acquired at the 6-m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences. It was shown that all three galaxies are peculiar late-type spirals in the state of ongoing interaction or merging.We discuss available photometric properties of the PRGs with spiral hosts and consider the Tully-Fisher relation for different types of PRGs. In agreement with Iodice et al. (2003), we have shown that true PRGs demonstrate similar to1/3 larger maximum rotation velocities than spiral galaxies of the same luminosity. Peculiar objects with forming polar structures satisfy, on average, the Tully-Fisher relation for disk galaxies but with large scatter.

AB - The results of B, V, R surface photometry of three polar-ring galaxies (PRGs) - A 0017+2212, UGC 1198, UGC 4385 - are presented. The data were acquired at the 6-m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences. It was shown that all three galaxies are peculiar late-type spirals in the state of ongoing interaction or merging.We discuss available photometric properties of the PRGs with spiral hosts and consider the Tully-Fisher relation for different types of PRGs. In agreement with Iodice et al. (2003), we have shown that true PRGs demonstrate similar to1/3 larger maximum rotation velocities than spiral galaxies of the same luminosity. Peculiar objects with forming polar structures satisfy, on average, the Tully-Fisher relation for disk galaxies but with large scatter.

KW - galaxies : individual : A 0017+2212, UGC 1198, UGC 4385

KW - galaxies : photometry

KW - galaxies : formation

KW - galaxies : structure

KW - NEAR-INFRARED PHOTOMETRY

KW - TULLY-FISHER RELATION

KW - INTERACTING GALAXIES

KW - IRAS OBSERVATIONS

KW - GLOBAL STRUCTURE

KW - SPIRAL GALAXIES

KW - DARK HALO

KW - KN-BANDS

KW - H-BANDS

KW - DISK

U2 - 10.1051/0004-6361:20031382

DO - 10.1051/0004-6361:20031382

M3 - статья

VL - 416

SP - 889

EP - 900

JO - ASTRONOMY & ASTROPHYSICS

JF - ASTRONOMY & ASTROPHYSICS

SN - 0004-6361

IS - 3

ER -

ID: 32201656