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Unveiling the Nature of Polar-ring Galaxies from Deep Imaging. / Mosenkov, Aleksandr V. ; Reshetnikov, Vladimir P. ; Skryabina, Maria N. ; Shakespear, Zacory.

в: Research in Astronomy and Astrophysics, Том 22, № 11, 115003, 11.2022.

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

Harvard

Mosenkov, AV, Reshetnikov, VP, Skryabina, MN & Shakespear, Z 2022, 'Unveiling the Nature of Polar-ring Galaxies from Deep Imaging', Research in Astronomy and Astrophysics, Том. 22, № 11, 115003. https://doi.org/10.1088/1674-4527/ac8d82

APA

Mosenkov, A. V., Reshetnikov, V. P., Skryabina, M. N., & Shakespear, Z. (2022). Unveiling the Nature of Polar-ring Galaxies from Deep Imaging. Research in Astronomy and Astrophysics, 22(11), [115003]. https://doi.org/10.1088/1674-4527/ac8d82

Vancouver

Mosenkov AV, Reshetnikov VP, Skryabina MN, Shakespear Z. Unveiling the Nature of Polar-ring Galaxies from Deep Imaging. Research in Astronomy and Astrophysics. 2022 Нояб.;22(11). 115003. https://doi.org/10.1088/1674-4527/ac8d82

Author

Mosenkov, Aleksandr V. ; Reshetnikov, Vladimir P. ; Skryabina, Maria N. ; Shakespear, Zacory. / Unveiling the Nature of Polar-ring Galaxies from Deep Imaging. в: Research in Astronomy and Astrophysics. 2022 ; Том 22, № 11.

BibTeX

@article{b192c28e9a324c209e838bf9ce66a9c8,
title = "Unveiling the Nature of Polar-ring Galaxies from Deep Imaging",
abstract = "General structural properties and low surface brightness tidal features hold important clues to the formation of galaxies. In this paper, we study a sample of polar-ring galaxies (PRGs) based on optical imaging from the Sloan Digital Sky Survey Stripe 82 and other deep surveys. We investigate the deepest images of candidates for PRGs to date. We carry out photometric decomposition on the host galaxies and associated polar structures that allows us to derive the structural properties of both components. We are able to detect very faint tidal structures around most PRGs in our sample. For several galaxies, we can directly observe the formation of the polar ring due to merging, which is manifested in debris of the victim galaxy and an arc-like polar structure made up of its material. In a few cases, we can discern signs of tidal accretion. The results obtained indicate that the gravitational interaction and merging of galaxies are the most plausible mechanisms for the formation of PRGs.",
keywords = "galaxies: structure, methods: data analysis, techniques: photometric",
author = "Mosenkov, {Aleksandr V.} and Reshetnikov, {Vladimir P.} and Skryabina, {Maria N.} and Zacory Shakespear",
note = "Publisher Copyright: {\textcopyright} 2022. National Astronomical Observatories, CAS and IOP Publishing Ltd.",
year = "2022",
month = nov,
doi = "10.1088/1674-4527/ac8d82",
language = "English",
volume = "22",
journal = "Research in Astronomy and Astrophysics",
issn = "1674-4527",
publisher = "IOP Publishing Ltd.",
number = "11",

}

RIS

TY - JOUR

T1 - Unveiling the Nature of Polar-ring Galaxies from Deep Imaging

AU - Mosenkov, Aleksandr V.

AU - Reshetnikov, Vladimir P.

AU - Skryabina, Maria N.

AU - Shakespear, Zacory

N1 - Publisher Copyright: © 2022. National Astronomical Observatories, CAS and IOP Publishing Ltd.

PY - 2022/11

Y1 - 2022/11

N2 - General structural properties and low surface brightness tidal features hold important clues to the formation of galaxies. In this paper, we study a sample of polar-ring galaxies (PRGs) based on optical imaging from the Sloan Digital Sky Survey Stripe 82 and other deep surveys. We investigate the deepest images of candidates for PRGs to date. We carry out photometric decomposition on the host galaxies and associated polar structures that allows us to derive the structural properties of both components. We are able to detect very faint tidal structures around most PRGs in our sample. For several galaxies, we can directly observe the formation of the polar ring due to merging, which is manifested in debris of the victim galaxy and an arc-like polar structure made up of its material. In a few cases, we can discern signs of tidal accretion. The results obtained indicate that the gravitational interaction and merging of galaxies are the most plausible mechanisms for the formation of PRGs.

AB - General structural properties and low surface brightness tidal features hold important clues to the formation of galaxies. In this paper, we study a sample of polar-ring galaxies (PRGs) based on optical imaging from the Sloan Digital Sky Survey Stripe 82 and other deep surveys. We investigate the deepest images of candidates for PRGs to date. We carry out photometric decomposition on the host galaxies and associated polar structures that allows us to derive the structural properties of both components. We are able to detect very faint tidal structures around most PRGs in our sample. For several galaxies, we can directly observe the formation of the polar ring due to merging, which is manifested in debris of the victim galaxy and an arc-like polar structure made up of its material. In a few cases, we can discern signs of tidal accretion. The results obtained indicate that the gravitational interaction and merging of galaxies are the most plausible mechanisms for the formation of PRGs.

KW - galaxies: structure

KW - methods: data analysis

KW - techniques: photometric

UR - https://www.mendeley.com/catalogue/f00b7ee6-8d87-35d7-88e9-3c93de4ae54f/

UR - http://www.scopus.com/inward/record.url?scp=85141264900&partnerID=8YFLogxK

U2 - 10.1088/1674-4527/ac8d82

DO - 10.1088/1674-4527/ac8d82

M3 - Article

VL - 22

JO - Research in Astronomy and Astrophysics

JF - Research in Astronomy and Astrophysics

SN - 1674-4527

IS - 11

M1 - 115003

ER -

ID: 99709391