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Visiting two objects in the field of the ring galaxy HRG 2302. / Faundez-Abans, M.; Reshetnikov, V. P.; de Oliveira-Abans, M.; Krabbe, A. C.; da Rocha-Poppe, P. C.; Fernandes-Martin, V. A.; Amores, E. B.; Freitas-Lemes, P.

в: Astronomy and Astrophysics, Том 574, 2015.

Результаты исследований: Научные публикации в периодических изданиях › статья

Harvard

Faundez-Abans, M, Reshetnikov, VP, de Oliveira-Abans, M, Krabbe, AC, da Rocha-Poppe, PC, Fernandes-Martin, VA, Amores, EB & Freitas-Lemes, P 2015, 'Visiting two objects in the field of the ring galaxy HRG 2302', Astronomy and Astrophysics, Том. 574. https://doi.org/10.1051/0004-6361/201425223

APA

Faundez-Abans, M., Reshetnikov, V. P., de Oliveira-Abans, M., Krabbe, A. C., da Rocha-Poppe, P. C., Fernandes-Martin, V. A., Amores, E. B., & Freitas-Lemes, P. (2015). Visiting two objects in the field of the ring galaxy HRG 2302. Astronomy and Astrophysics, 574. https://doi.org/10.1051/0004-6361/201425223

Vancouver

Faundez-Abans M, Reshetnikov VP, de Oliveira-Abans M, Krabbe AC, da Rocha-Poppe PC, Fernandes-Martin VA и пр. Visiting two objects in the field of the ring galaxy HRG 2302. Astronomy and Astrophysics. 2015;574. https://doi.org/10.1051/0004-6361/201425223

Author

Faundez-Abans, M. ; Reshetnikov, V. P. ; de Oliveira-Abans, M. ; Krabbe, A. C. ; da Rocha-Poppe, P. C. ; Fernandes-Martin, V. A. ; Amores, E. B. ; Freitas-Lemes, P. / Visiting two objects in the field of the ring galaxy HRG 2302. в: Astronomy and Astrophysics. 2015 ; Том 574.

BibTeX

@article{05137c1b5c354705a88162de263f9b92,
title = "Visiting two objects in the field of the ring galaxy HRG 2302",
abstract = "Aims. We investigate the nature of two galaxies that are located in the field of the ring galaxy HRG 2302. Methods. This study is based on direct BVRI imaging and long-slit spectrophotometric data in the range of 4000−9500 {\AA} obtained with the 1.6 m telescope of the Observat{\'o}rio do Pico dos Dias, Brazil. The spectra were used to determine the radial velocity. Results. The primary objective of the retrieval of the photometric data was to identify the fine structures of objects H and I. In addition, we performed image processing and made a photometric analysis to obtain the integrated standard BVRI magnitudes. The contour maps show evidence of material connecting both galaxies, suggesting that they might be interacting close companions. We estimated redshifts of z = 0.0689 and z = 0.0692. The spectra of the two galaxies resemble those of an early-type galaxy. The fact that the objects have a small radial-velocity difference and the structures around object I suggest an ongoing tidal interaction between the two",
keywords = "galaxies, interactions, peculiar",
author = "M. Faundez-Abans and Reshetnikov, {V. P.} and {de Oliveira-Abans}, M. and Krabbe, {A. C.} and {da Rocha-Poppe}, {P. C.} and Fernandes-Martin, {V. A.} and Amores, {E. B.} and P. Freitas-Lemes",
year = "2015",
doi = "10.1051/0004-6361/201425223",
language = "English",
volume = "574",
journal = "ASTRONOMY & ASTROPHYSICS",
issn = "0004-6361",
publisher = "EDP Sciences",

}

RIS

TY - JOUR

T1 - Visiting two objects in the field of the ring galaxy HRG 2302

AU - Faundez-Abans, M.

AU - Reshetnikov, V. P.

AU - de Oliveira-Abans, M.

AU - Krabbe, A. C.

AU - da Rocha-Poppe, P. C.

AU - Fernandes-Martin, V. A.

AU - Amores, E. B.

AU - Freitas-Lemes, P.

PY - 2015

Y1 - 2015

N2 - Aims. We investigate the nature of two galaxies that are located in the field of the ring galaxy HRG 2302. Methods. This study is based on direct BVRI imaging and long-slit spectrophotometric data in the range of 4000−9500 Å obtained with the 1.6 m telescope of the Observatório do Pico dos Dias, Brazil. The spectra were used to determine the radial velocity. Results. The primary objective of the retrieval of the photometric data was to identify the fine structures of objects H and I. In addition, we performed image processing and made a photometric analysis to obtain the integrated standard BVRI magnitudes. The contour maps show evidence of material connecting both galaxies, suggesting that they might be interacting close companions. We estimated redshifts of z = 0.0689 and z = 0.0692. The spectra of the two galaxies resemble those of an early-type galaxy. The fact that the objects have a small radial-velocity difference and the structures around object I suggest an ongoing tidal interaction between the two

AB - Aims. We investigate the nature of two galaxies that are located in the field of the ring galaxy HRG 2302. Methods. This study is based on direct BVRI imaging and long-slit spectrophotometric data in the range of 4000−9500 Å obtained with the 1.6 m telescope of the Observatório do Pico dos Dias, Brazil. The spectra were used to determine the radial velocity. Results. The primary objective of the retrieval of the photometric data was to identify the fine structures of objects H and I. In addition, we performed image processing and made a photometric analysis to obtain the integrated standard BVRI magnitudes. The contour maps show evidence of material connecting both galaxies, suggesting that they might be interacting close companions. We estimated redshifts of z = 0.0689 and z = 0.0692. The spectra of the two galaxies resemble those of an early-type galaxy. The fact that the objects have a small radial-velocity difference and the structures around object I suggest an ongoing tidal interaction between the two

KW - galaxies

KW - interactions

KW - peculiar

U2 - 10.1051/0004-6361/201425223

DO - 10.1051/0004-6361/201425223

M3 - Article

VL - 574

JO - ASTRONOMY & ASTROPHYSICS

JF - ASTRONOMY & ASTROPHYSICS

SN - 0004-6361

ER -

ID: 3926143