The H I Parkes Zone of Avoidance Survey:: The northern extension

被引:37
作者
Donley, JL
Staveley-Smith, L
Kraan-Korteweg, RC
Islas-Islas, JM
Schröder, A
Henning, PA
Koribalski, B
Mader, S
Stewart, I
机构
[1] CSIRO, Australia Telescope Natl Facil, Epping, NSW 1710, Australia
[2] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
[3] Univ Guanajuato, Dept Astron, Guanajuato 36000, GTO, Mexico
[4] Univ Leicester, Dept Phys & Astron, Leicester LE1 7RH, Leics, England
[5] Univ New Mexico, Inst Astrophys, Albuquerque, NM 87131 USA
关键词
galaxies : distances and redshifts; galaxies : fundamental parameters; large-scale structure of universe; surveys;
D O I
10.1086/426320
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the results of the northern extension of the H I Parkes Zone of Avoidance Survey, a blind H I survey utilizing the multibeam receiver on the Parkes 64 m telescope. In the two regions studied here, l = 36degrees - 52degrees and l = 196degrees - 212degrees, \b\ less than or equal to 5degrees, we have detected 77 H I galaxies, 20 of which have been previously detected in H I. The survey has a median rms noise of 6.0 mJy beam(-1) and is complete to a mean flux density of 22 mJy. We have searched for multiwavelength counterparts to the 77 galaxies detected here: 19, 27, and 11 have a likely optical, 2MASS, and IRAS cataloged counterpart, respectively. A further 16 galaxies have likely visible counterparts on the Digitized Sky Survey. The detection of these 77 galaxies allows a closer inspection of the large-scale structures in these regions. We see several filaments crossing the Galactic plane, one of which appears to be the continuation of a sine-wave-like feature that can be traced across the whole southern sky. An analysis of the H I mass function suggests that the regions studied here may be underdense. One particularly noteworthy galaxy is HIZOA J0630+08 (l, b = 203degrees, - 0.degrees9) with a velocity of 367 +/- 1 km s(-1). We suggest that it belongs to the nearby Orion Group, which includes a small number of dwarf galaxies. The newly detected galaxies improve our understanding of the properties of several voids, such as the Orion, Gemini, and Canis Major voids.
引用
收藏
页码:220 / 238
页数:19
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