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A New 2MASS/2df Selected Sample of Pairs of Galaxies and Calibration of Merging Rate in the Local Universe |
| SUN Yan-Chun1;C. K. XU2;HE Xiang-Tao1 |
| 1Department of Astronomy, Beijing Normal University, Beijing 100875
2Infrared Processing and Analysis Center, Jet Propulsion Laboratory, California Institute of Technology 100-22, Pasadena, CA 91125, USA |
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| Cite this article: |
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SUN Yan-Chun, C. K. XU, HE Xiang-Tao 2003 Chin. Phys. Lett. 20 1652-1655 |
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Abstract We present a new sample of 37 close major-merger galaxy pairs, selected from the 2-degree field redshift survey of the two-micron all-sky survey (2MASS) galaxies. The selection criteria for our near-infrared pairs are more closely related to galaxy mass (a very important parameter in galaxy evolution models) than those for optical selected samples. Our sample benefits enormously from the high homogeneity and accuracy of the 2MASS database, and false matchings are minimized by the essentially three-dimensional selection procedure. Taking into account the biases, we find that 1.96 (±0.4)% of galaxies are in close major-merger pairs. This indicates a local merging rate of 1.0%, in good agreement with the results in recent studies of optical selected pairs in the local universe. The results derived with our sample have high confidence.
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| Keywords:
98.65.At
98.62.Py
98.62.Ai
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Published: 01 September 2003
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| PACS: |
98.65.At
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(Interacting galaxies; galaxy pairs, and triples)
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98.62.Py
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(Distances, redshifts, radial velocities; spatial distribution of galaxies)
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98.62.Ai
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(Origin, formation, evolution, age, and star formation)
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