2024A&A...681L..15M


Query : 2024A&A...681L..15M

2024A&A...681L..15M - Astronomy and Astrophysics, volume 681L15 (2024/1-1)

The occurrence rate of galaxies with polar structures may be significantly underestimated.

MOSENKOV A.V., BAHR S.K.H., RESHETNIKOV V.P., SHAKESPEAR Z. and SMIRNOV D.V.

Abstract (from CDS):

Polar-ring galaxies are photometrically and kinematically decoupled systems that are highly inclined to the major axis of the host. These galaxies have been explored since the 1970s, but the rarity of these systems has made such systematic studies difficult. However, over 250 good candidates have been identified. In this work, we examine a sample of over 18 000 galaxies from the Sloan Digital Sky Survey (SDSS) Stripe 82 for the presence of galaxies with polar structures. Using deep SDSS Stripe 82, DESI Legacy Imaging Surveys, and Hyper Suprime-Cam Subaru Strategic Program, we selected 53 good candidate galaxies with photometrically decoupled polar rings, 9 galaxies with polar halos, 6 galaxies with polar bulges, and 34 possibly forming polar-ring galaxies, versus 13 polar-ring candidates previously selected in Stripe 82. Our results suggest that the occurrence rate of galaxies with polar structures may be significantly underestimated, as revealed by the deep observations, and may amount to 1-3% of non-dwarf galaxies.

Abstract Copyright: © The Authors 2024

Journal keyword(s): galaxies: elliptical and lenticular, cD - galaxies: evolution - galaxies: formation - galaxies: structure

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 M 104 LIN 12 39 59.43185902 -11 37 22.9961800 9.51 9.55 8.00 8.05   ~ 1465 2
2 NGC 4632 EmG 12 42 31.9886669016 -00 04 57.071456184   12.5   12.4 11.9 ~ 177 0
3 NGC 6156 AGN 16 34 52.5448490040 -60 37 07.867951500   12.30   11.05 12.0 ~ 85 0

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