Optical identifications of 230 HIPASS radio sources
被引:0
作者:
I. D. Karachentsev
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机构:Russian Academy of Sciences,Special Astrophysical Observatory
I. D. Karachentsev
D. I. Makarov
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h-index: 0
机构:Russian Academy of Sciences,Special Astrophysical Observatory
D. I. Makarov
V. E. Karachentseva
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机构:Russian Academy of Sciences,Special Astrophysical Observatory
V. E. Karachentseva
O. V. Melnik
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机构:Russian Academy of Sciences,Special Astrophysical Observatory
O. V. Melnik
机构:
[1] Russian Academy of Sciences,Special Astrophysical Observatory
[2] Observatoire de Lyon,Astronomical Observatory
[3] Kiev National University,undefined
来源:
Astronomy Letters
|
2008年
/
34卷
关键词:
dwarf galaxies;
galaxy evolution;
interstellar gas in galaxies;
95.80.+p;
98.52.Wz;
98.56.Wm;
98.62.Py;
98.62.Ve;
D O I:
暂无
中图分类号:
学科分类号:
摘要:
We present the coordinates, apparent magnitudes, and morphological types for 230 galaxies presumably identified with HIPASS (HI Parkes All-Sky Survey) sources. The new optical counterparts of the HIPASS sources follow the well-known statistical relationships between the hydrogen mass, luminosity, and type of galaxies. Low-surface-brightness galaxies constitute a significant fraction among these objects. The median value of the hydrogen mass-to-luminosity ratio for them is a factor of 2 or 3 higher than that for bright HIPASS galaxies, reaching 1.7M⊙/L⊙. A number of our objects are located near the boundary log(MHI/LB) = 0.2(MB + 20) that defines the zone of gravitational stability of disk galaxies against large-scale star formation.