The multiwavelength Tully-Fisher relation with spatially resolved H I kinematics

Anastasia A. Ponomareva; Marc A. W. Verheijen; Reynier F. Peletier; Albert Bosma

doi:10.1093/mnras/stx1018

The multiwavelength Tully-Fisher relation with spatially resolved H I kinematics

Anastasia A. Ponomareva, Marc A. W. Verheijen, Reynier F. Peletier, Albert Bosma

Astronomy

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Abstract

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 μm) and of spatially resolved H I kinematics. We use these data together with three kinematic measures (WI_{50}, Vmax and Vflat) extracted from the global H I profiles or H I rotation curves, so as to construct 36 correlations allowing us to select the one with the least scatter. We introduce a tightness parameter σ⊥ 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 μm photometric band together with the Vflat parameter extracted from the H I rotation curve.

Original language	English
Pages (from-to)	2387-2400
Number of pages	14
Journal	Monthly Notices of the Royal Astronomical Society
Volume	469
Issue number	2
DOIs	https://doi.org/10.1093/mnras/stx1018
Publication status	Published - 1-Aug-2017

Keywords

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

Access to Document

10.1093/mnras/stx1018

The multiwavelength TullyFinal publisher's version, 1.73 MBLicence: Unspecified

http://adsabs.harvard.edu/abs/2017MNRAS.469.2387P

Cite this

@article{15f105d03cbc450ab9d2275e6e504a94,

title = "The multiwavelength Tully-Fisher relation with spatially resolved H I kinematics",

abstract = "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 μm) and of spatially resolved H I kinematics. We use these data together with three kinematic measures (WI_{50}, Vmax and Vflat) extracted from the global H I profiles or H I rotation curves, so as to construct 36 correlations allowing us to select the one with the least scatter. We introduce a tightness parameter σ⊥ 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 μm photometric band together with the Vflat parameter extracted from the H I rotation curve.",

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

author = "Ponomareva, {Anastasia A.} and Verheijen, {Marc A. W.} and Peletier, {Reynier F.} and Albert Bosma",

year = "2017",

month = aug,

day = "1",

doi = "10.1093/mnras/stx1018",

language = "English",

volume = "469",

pages = "2387--2400",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

publisher = "Oxford University Press",

number = "2",

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TY - JOUR

T1 - The multiwavelength Tully-Fisher relation with spatially resolved H I kinematics

AU - Ponomareva, Anastasia A.

AU - Verheijen, Marc A. W.

AU - Peletier, Reynier F.

AU - Bosma, Albert

PY - 2017/8/1

Y1 - 2017/8/1

N2 - 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 μm) and of spatially resolved H I kinematics. We use these data together with three kinematic measures (WI_{50}, Vmax and Vflat) extracted from the global H I profiles or H I rotation curves, so as to construct 36 correlations allowing us to select the one with the least scatter. We introduce a tightness parameter σ⊥ 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 μm photometric band together with the Vflat parameter extracted from the H I rotation curve.

AB - 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 μm) and of spatially resolved H I kinematics. We use these data together with three kinematic measures (WI_{50}, Vmax and Vflat) extracted from the global H I profiles or H I rotation curves, so as to construct 36 correlations allowing us to select the one with the least scatter. We introduce a tightness parameter σ⊥ 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 μm photometric band together with the Vflat parameter extracted from the H I rotation curve.

KW - galaxies: fundamental parameters

KW - galaxies: kinematics and dynamics

KW - galaxies: photometry

KW - SURFACE PHOTOMETRY

KW - DISTANCE SCALE

KW - URSA-MAJOR CLUSTER

KW - MORPHOLOGICAL TYPE DEPENDENCE

KW - STELLAR MASS DISTRIBUTIONS

KW - DECLINING ROTATION CURVES

KW - VELOCITY-WIDTH RELATION

KW - SPIRAL GALAXIES

KW - DWARF GALAXIES

KW - DARK-MATTER

U2 - 10.1093/mnras/stx1018

DO - 10.1093/mnras/stx1018

M3 - Article

VL - 469

SP - 2387

EP - 2400

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 2

ER -