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Galaxy Triplets in the Local Supercluster

期刊

ASTROPHYSICAL BULLETIN
卷 64, 期 1, 页码 24-49

出版社

MAIK NAUKA/INTERPERIODICA/SPRINGER
DOI: 10.1134/S1990341309010027

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资金

  1. Russian Foundation for Basic Research [07 -02 -00005, 08 -02 -00627, 0-02-00792]
  2. Deutsche Forschungsgemeinschaft and Russian Foundation [06 02-04017]

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We report a catalog of 168 galaxy triplets with line-of-sight velocities V-LG < 3500 km/s identified using a percolation criterion, which takes individual properties of galaxies into account. The catalog contains the line-of-sight velocities, K-band magnitudes, and morphological types of galaxies. Our sample of galaxy triplets is characterized by the median values of the line-of-sight velocity dispersion, projected harmonic radius, and crossing time of 40 km/s, 155 kpc, and 3 Gyr, respectively. The median projected mass and K-band luminosity of our triplets are equal to 5 x 10(11)M(circle dot) and 15M(circle dot)/L-circle dot, respectively, with the uncertainty of these parameters due mostly to the errors of radial-velocity measurements. The basic properties of triple systems in the Local Supercluster are compared to those of more distant isolated triplets from the KTG and KTS samples. The fraction of triplet members among all galaxies is found be more than 5%.

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