Standard

UGC 5119: A Galaxy with a Stellar Polar Ring? / Yakovleva, V. A.; Karataeva, G. M.

в: Astronomy Letters, Том 30, № 8, 2004, стр. 519-526.

Результаты исследований: Научные публикации в периодических изданияхстатьяРецензирование

Harvard

APA

Vancouver

Author

Yakovleva, V. A. ; Karataeva, G. M. / UGC 5119: A Galaxy with a Stellar Polar Ring?. в: Astronomy Letters. 2004 ; Том 30, № 8. стр. 519-526.

BibTeX

@article{9f5a2d6504914d02906bd892daec31dd,
title = "UGC 5119: A Galaxy with a Stellar Polar Ring?",
abstract = "We present our photometric BVRc observations of UGC 5119, a candidate polar-ring galaxy. We have determined its absolute magnitude, M0,B = -20.3 mag, and total color indices, (B-V)t0 = +0.73 +/- 0.10 mag and (V-Rc)t0 = +0.54 +/- 0.10 mag. A Fourier analysis of the shape of its isophotes shows that UGC 5119 is most likely an elliptical galaxy with a disk component in the central part and a {"}boxy{"} feature on the periphery. At distances larger than 8 arcsec, the galaxy exhibits a turn of its major axis and a change in the phase of the fourth harmonic. Assuming the position angle of the major axis to be constant, a stellar ringlike structure is distinguished in the galaxy. The age of the ring stars is the same as that of the stars in the host galaxy. The distinguished ringlike structure cannot be attributed to typical polar rings rich in gas and in young stars.",
author = "Yakovleva, {V. A.} and Karataeva, {G. M.}",
year = "2004",
doi = "10.1134/1.1784493",
language = "English",
volume = "30",
pages = "519--526",
journal = "Astronomy Letters",
issn = "1063-7737",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "8",

}

RIS

TY - JOUR

T1 - UGC 5119: A Galaxy with a Stellar Polar Ring?

AU - Yakovleva, V. A.

AU - Karataeva, G. M.

PY - 2004

Y1 - 2004

N2 - We present our photometric BVRc observations of UGC 5119, a candidate polar-ring galaxy. We have determined its absolute magnitude, M0,B = -20.3 mag, and total color indices, (B-V)t0 = +0.73 +/- 0.10 mag and (V-Rc)t0 = +0.54 +/- 0.10 mag. A Fourier analysis of the shape of its isophotes shows that UGC 5119 is most likely an elliptical galaxy with a disk component in the central part and a "boxy" feature on the periphery. At distances larger than 8 arcsec, the galaxy exhibits a turn of its major axis and a change in the phase of the fourth harmonic. Assuming the position angle of the major axis to be constant, a stellar ringlike structure is distinguished in the galaxy. The age of the ring stars is the same as that of the stars in the host galaxy. The distinguished ringlike structure cannot be attributed to typical polar rings rich in gas and in young stars.

AB - We present our photometric BVRc observations of UGC 5119, a candidate polar-ring galaxy. We have determined its absolute magnitude, M0,B = -20.3 mag, and total color indices, (B-V)t0 = +0.73 +/- 0.10 mag and (V-Rc)t0 = +0.54 +/- 0.10 mag. A Fourier analysis of the shape of its isophotes shows that UGC 5119 is most likely an elliptical galaxy with a disk component in the central part and a "boxy" feature on the periphery. At distances larger than 8 arcsec, the galaxy exhibits a turn of its major axis and a change in the phase of the fourth harmonic. Assuming the position angle of the major axis to be constant, a stellar ringlike structure is distinguished in the galaxy. The age of the ring stars is the same as that of the stars in the host galaxy. The distinguished ringlike structure cannot be attributed to typical polar rings rich in gas and in young stars.

U2 - 10.1134/1.1784493

DO - 10.1134/1.1784493

M3 - Article

VL - 30

SP - 519

EP - 526

JO - Astronomy Letters

JF - Astronomy Letters

SN - 1063-7737

IS - 8

ER -

ID: 5190945