The multiwavelength Tully-Fisher relation with spatially resolved HI kinematics

被引：51

作者：

Ponomareva, Anastasia A. ^{[1
,2
]}

Verheijen, Marc A. W. ^{[2
,3
]}

Peletier, Reynier F. ^{[2
]}

Bosma, Albert ^{[4
]}

机构：

[1] Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2611, Australia

[2] Univ Groningen, Kapteyn Astron Inst, Postbus 800, NL-9700 AV Groningen, Netherlands

[3] TIFR, Natl Ctr Radio Astrophys, Adjunct Fac, Pune 411007, Maharashtra, India

[4] Aix Marseille Univ, CNRS, UMR 7326, LAM, F-13388 Marseille, France

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2017年 / 469卷 / 02期

基金：

美国国家航空航天局;

关键词：

galaxies: fundamental parameters; galaxies: kinematics and dynamics; galaxies: photometry; URSA-MAJOR CLUSTER; MORPHOLOGICAL TYPE DEPENDENCE; STELLAR MASS DISTRIBUTIONS; DECLINING ROTATION CURVES; VELOCITY-WIDTH RELATION; SPIRAL GALAXIES; DWARF GALAXIES; DARK-MATTER; SURFACE PHOTOMETRY; DISTANCE SCALE;

D O I：

10.1093/mnras/stx1018

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In this paper, we investigate the statistical properties of the Tully-Fisher relation (TFr) for a sample of 32 galaxies with measured distances from the Cepheid period-luminosity relation and/or TRGB stars. We take advantage of panchromatic photometry in 12 bands (from FUV to 4.5 mu m) and of spatially resolved HI kinematics. We use these data together with three kinematic measures (W-50(i), V-max and V-flat) extracted from the global HI profiles or HI rotation curves, so as to construct 36 correlations allowing us to select the one with the least scatter. We introduce a tightness parameter sigma (perpendicular to). of the TFr, in order to obtain a slope-independent measure of the goodness of fit. We find that the tightest correlation occurs when we select the 3.6 mu m photometric band together with the V-flat parameter extracted from the HI rotation curve.

引用

页码：2387 / 2400

页数：14

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