Distances and peculiar velocities of spiral galaxies in the 2MFGC and SFI++ samples

We compare infrared Tully-Fisher (TF) distances and peculiar velocities derived for spiral galaxies from the two largest datasets: the 2MASS selected Flat Galaxy Catalog 2MFGC and the Arecibo General Catalog with I-band photometry, SFI++. These samples contain peculiar velocities for ~3000 and ~4000...

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Published inAstrophysics Vol. 52; no. 3; pp. 335 - 349
Main Authors Kudrya, Yu. N., Karachentseva, V. E., Karachentsev, I. D., Mitronova, S. N., Huchtmeier, W. K.
Format Journal Article
LanguageEnglish
Published Boston Springer US 01.07.2009
Springer Nature B.V
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Summary:We compare infrared Tully-Fisher (TF) distances and peculiar velocities derived for spiral galaxies from the two largest datasets: the 2MASS selected Flat Galaxy Catalog 2MFGC and the Arecibo General Catalog with I-band photometry, SFI++. These samples contain peculiar velocities for ~3000 and ~4000 objects, respectively. Based on a sub-sample of ~1000 common very inclined galaxies, we reach the following conclusions. Irrespective of high (SFI++) or low (2MFGC) quality of the photometric data used, both the samples have ~10% fraction of galaxies deviating considerably from the main body of the TF relation. After their deletion, the standard TF scatter drops to 0 m .47 (2MFGC) and 0 m .40 (SFI++). The TF distances, derived from two samples, demonstrate a high degree of mutual agreement with a correlation coefficient ρ = +0 . 95 and σ( H 0 r ) = 837 km/s. Peculiar velocities of the galaxies are also correlated with ρ = 0 . 56−0 . 59 and σ( V pec ) = 610 V pec km/s. We find that the bulk motion of the 2MFGC and SFI++ galaxies on a typical scale of H 0 r ≈ 5700 km/s can be represented by a dipole solution with the amplitude V = (297 ± 23) km/s directed towards { l = 292 0 ± 4 0 , b = −12 0 ± 3 0 }, being only slightly sensitive to different modifications of the TF relaton.
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ISSN:0571-7256
1573-8191
DOI:10.1007/s10511-009-9070-8