A deep near-infrared survey around the giant radio galaxy PKS 1343-601

被引:19
|
作者
Nagayama, T [1 ]
Woudt, PA
Nagashima, C
Nakajima, Y
Kato, D
Kurita, M
Nagata, T
Nakaya, H
Tamura, M
Sugitani, K
Wakamatsu, K
Sato, S
机构
[1] Nagoya Univ, Dept Astrophys, Chikusa Ku, Nagoya, Aichi 4648602, Japan
[2] Univ Cape Town, Dept Astron, ZA-7700 Rondebosch, South Africa
[3] Natl Astron Observ Japan, Tokyo 1818858, Japan
[4] Natl Astron Observ Japan, Subaru Telescope, Hilo, HI 96720 USA
[5] Nagoya City Univ, Inst Nat Sci, Mizuho Ku, Nagoya, Aichi 4678501, Japan
[6] Gifu Univ, Fac Engn, Gifu 5011193, Japan
关键词
surveys; dust; extinction; galaxies : clusters : general; galaxies : fundamental parameters; galaxies : individual : PKS 1343-601; infrared : galaxies;
D O I
10.1111/j.1365-2966.2004.08277.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the results of a deep near-infrared survey of a 36 x 36 arcmin(2) region centred on the giant elliptical radio galaxy PKS 1343-601, suggested to be the core of an unknown rich cluster located at the low Galactic latitude of b = 1.degrees73 in the Great Attractor (GA) region. 19 obvious galaxies and 38 galaxy candidates have been detected; only three of them were previously identified as a galaxy. The total Galactic extinction A(K) towards our survey area is estimated to be 0.6-0.8 mag from the J-K colour of foreground giants. This is systematically lower by about 0.4 mag than A(K) taken from the IRAS/DIRBE extinction map. The number density of galaxies brighter than an extinction-corrected Ks band magnitude of 13 is 42 galaxies deg(-2), five times as high as the overall average in the GA region. However, the number of galaxies within the central 270-kpc radius is less than that of the Norma, Pavo and Centaurus clusters in the GA region. We found no evidence that a rich cluster is associated with PKS 1343-601.
引用
收藏
页码:980 / 990
页数:11
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