Tully-Fisher relation distances
E517969
Tully-Fisher relation distances are galaxy distance measurements derived from the empirical correlation between a spiral galaxy’s luminosity and its rotational velocity.
All labels observed (2)
| Label | Occurrences |
|---|---|
| Tully–Fisher relation | 3 |
| Tully-Fisher relation distances canonical | 1 |
How this entity was disambiguated
This entity first appeared as the object of triple T5410706 — resolving that mention is where its identity was fixed. The disambiguator weighed these candidate entities and picked the highlighted one (or “None”, minting a new entity). This is how homonymy is resolved: the same surface form can point to different entities.
Target entity: Tully-Fisher relation distances Context triple: [Cosmicflows-2 data set, includes, Tully-Fisher relation distances]
-
A.
A Relation between Distance and Radial Velocity among Extra-Galactic Nebulae
"A Relation between Distance and Radial Velocity among Extra-Galactic Nebulae" is Edwin Hubble’s landmark 1929 paper that established the linear relationship between galaxies’ distances and their recessional velocities, providing the first strong evidence for the expanding universe.
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B.
Faber–Jackson relation paper
The Faber–Jackson relation paper is a landmark astrophysics publication that established a correlation between the luminosity and stellar velocity dispersion of elliptical galaxies, providing key insights into their structure and evolution.
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C.
Faber–Jackson relation
The Faber–Jackson relation is an empirical correlation in astronomy that links the luminosity of an elliptical galaxy to the velocity dispersion of its stars, providing a key tool for estimating galactic distances and masses.
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D.
Tolman surface brightness test
The Tolman surface brightness test is an observational cosmology method that checks whether the universe is expanding by examining how the surface brightness of distant galaxies diminishes with redshift.
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E.
Zwicky catalog of galaxies
The Zwicky catalog of galaxies is an influential astronomical catalog compiled by Swiss astronomer Fritz Zwicky that systematically lists and classifies thousands of galaxies and galaxy clusters.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
Target entity: Tully-Fisher relation distances Target entity description: Tully-Fisher relation distances are galaxy distance measurements derived from the empirical correlation between a spiral galaxy’s luminosity and its rotational velocity.
-
A.
A Relation between Distance and Radial Velocity among Extra-Galactic Nebulae
"A Relation between Distance and Radial Velocity among Extra-Galactic Nebulae" is Edwin Hubble’s landmark 1929 paper that established the linear relationship between galaxies’ distances and their recessional velocities, providing the first strong evidence for the expanding universe.
-
B.
Faber–Jackson relation paper
The Faber–Jackson relation paper is a landmark astrophysics publication that established a correlation between the luminosity and stellar velocity dispersion of elliptical galaxies, providing key insights into their structure and evolution.
-
C.
Faber–Jackson relation
The Faber–Jackson relation is an empirical correlation in astronomy that links the luminosity of an elliptical galaxy to the velocity dispersion of its stars, providing a key tool for estimating galactic distances and masses.
-
D.
Tolman surface brightness test
The Tolman surface brightness test is an observational cosmology method that checks whether the universe is expanding by examining how the surface brightness of distant galaxies diminishes with redshift.
-
E.
Zwicky catalog of galaxies
The Zwicky catalog of galaxies is an influential astronomical catalog compiled by Swiss astronomer Fritz Zwicky that systematically lists and classifies thousands of galaxies and galaxy clusters.
- F. None of above. chosen
Statements (47)
| Predicate | Object |
|---|---|
| instanceOf |
extragalactic distance indicator
ⓘ
secondary distance indicator ⓘ |
| appliesTo | spiral galaxies ⓘ |
| assume |
a universal Tully-Fisher relation for a given band
ⓘ
rotational velocity traces total mass ⓘ |
| basedOn | Tully-Fisher relation NERFINISHED ⓘ |
| calibratedIn |
nearby galaxy clusters
ⓘ
the Local Group outskirts ⓘ |
| contributeTo |
constraints on local Hubble flow
ⓘ
studies of galaxy scaling relations ⓘ |
| dependsOn |
choice of photometric band
ⓘ
galaxy inclination correction ⓘ internal extinction correction ⓘ k-correction for magnitudes ⓘ |
| implementedWith |
21-cm HI line width measurements
ⓘ
optical emission line rotation curves ⓘ |
| notWellSuitedFor |
elliptical galaxies
ⓘ
irregular galaxies with disturbed kinematics ⓘ |
| oftenUse |
I-band photometry
ⓘ
near-infrared photometry ⓘ |
| relatedTo |
Faber-Jackson relation distances
ⓘ
Fundamental Plane distances ⓘ baryonic Tully-Fisher relation distances ⓘ |
| requiresCalibrationWith |
Cepheid variable distances
ⓘ
Type Ia supernova distances ⓘ primary distance indicators ⓘ |
| sensitiveTo |
galaxy inclination uncertainties
ⓘ
galaxy morphological type ⓘ line width measurement errors ⓘ zero-point calibration errors ⓘ |
| systematicUncertaintiesInclude |
Malmquist bias
NERFINISHED
ⓘ
environmental effects on galaxy properties ⓘ selection biases ⓘ |
| typicalRandomUncertainty | about 15 to 20 percent in distance ⓘ |
| usedBy |
cosmological flow surveys
ⓘ
distance scale calibration projects ⓘ |
| usedFor |
estimating the Hubble constant
ⓘ
mapping large-scale structure ⓘ measuring distances in the nearby universe ⓘ measuring distances to cluster spiral galaxies ⓘ measuring distances to field spiral galaxies ⓘ peculiar velocity studies ⓘ |
| usesCorrelationBetween | galaxy luminosity and rotational velocity ⓘ |
| usesObservable |
galaxy apparent magnitude
ⓘ
galaxy rotational line width ⓘ |
| validFor | disk-dominated galaxies ⓘ |
| yields | galaxy distance modulus ⓘ |
How these facts were elicited
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Subject: Tully-Fisher relation distances Description of subject: Tully-Fisher relation distances are galaxy distance measurements derived from the empirical correlation between a spiral galaxy’s luminosity and its rotational velocity.
Referenced by (4)
Full triples — surface form annotated when it differs from this entity's canonical label.