A catalogue of galaxies behind the southern Milky Way ?: II.: The Crux and Great Attractor regions (l≈289° to 338°)

被引:35
|
作者
Woudt, PA [1 ]
Kraan-Korteweg, RC
机构
[1] Univ Cape Town, Dept Astron, ZA-7700 Rondebosch, South Africa
[2] Univ Guanajuato, Dept Astron, Guanajuato 36000, Mexico
关键词
catalogues; surveys; ISM; dust; extinction; galaxies : fundamental parameters; cosmology : large-scale structure of the Universe;
D O I
10.1051/0004-6361:20011455
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this second paper of the catalogue series of galaxies behind the southern Milky Way, we report on the deep optical galaxy search in the Crux region (289 degrees less than or equal to l less than or equal to 318 degrees and -10 degrees less than or equal to b less than or equal to 10 degrees) and the Great Attractor region (316 degrees less than or equal to l less than or equal to 338 degrees and -10 degrees less than or equal to b less than or equal to 10 degrees). The galaxy catalogues are presented, a brief description of the galaxy search given, as well as a discussion on the distribution and characteristics of the uncovered galaxies. A total of 8182 galaxies with major diameters D greater than or similar to 0.'2 were identified in this similar to 850 square degree area: 3759 galaxies in the Crux region and 4423 galaxies in the Great Attractor region. Of the 8182 galaxies, 229 (2.8%) were catalogued before in the optical (3 in radio) and 251 galaxies have a reliable (159), or likely (92) cross-identification in the IRAS Point Source Catalogue (3.1%). A number of prominent overdensities and filaments of galaxies are identified. They are not correlated with the Galactic foreground extinction and hence indicative of extragalactic large-scale structures. Redshifts obtained at the South African Astronomical Observatory (SAAO) for 518 of the newly catalogued galaxies in the Crux and Great Attractor regions (Fairall et al. 1998; Woudt et al. 1999) confirm distinct voids and clusters in the area here surveyed. With this optical galaxy search, we have reduced the width of the optical "Zone of Avoidance" for galaxies with extinction-corrected diameters larger than 1.3 arcmin from extinction levels A(B) greater than or equal to 1.(m)0 to A(B) greater than or equal to 3.(m)0: the remaining optical Zone of Avoidance is now limited by \b\ less than or similar to 3 degrees (see Fig. 16).
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页码:441 / 459
页数:19
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