期刊
ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS
卷 37, 期 3, 页码 171-180出版社
PLEIADES PUBLISHING INC
DOI: 10.1134/S1063773711030042
关键词
galaxies; interacting galaxies; morphology; kinematics
资金
- Russian Foundation for Basic Research [09-02-00968]
We present the results of our observational study of two candidates for polar-ring galaxies (PRGs). Both objects, A2330-3751 and SDSS J000911.57-003654.7, are giant edge-on galaxies with large-scale structures resembling polar rings observed along their minor axes. The optical diameter of the putative ring reaches 60 kpc in A2330-3751 and 18 kpc in SDSS J000911.57-003654.7. To estimate the space density of PRGs, we have constructed their luminosity function in the range of B-band absolute magnitudes from -17 (center dot) (m) 5 to -21 (center dot) (m) 5. We have found that similar to 10(-3) of the nearby galaxies exhibit polar structures. Polar rings around early-type (E/S0) galaxies are encountered approximately a factor of 3 more frequently than those around spiral ones. According to our estimates, similar to 20-30 PRGs in which large-scale rings are seen almost face-on must be observed among relatively bright galaxies (B a parts per thousand currency sign 15 (m) ).
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