Tully-Fisher relation
Definition: An empirical correlation between a disk galaxy's luminosity or baryonic mass and characteristic rotation speed.
Why it matters here: It constrains galaxy formation and can provide relative distances when calibrated.
Relationship: A common form is \(L\propto v_c^\alpha\), with slope and scatter depending on observable choices.
Limitation or common confusion: It is a statistical relation, not an exact law for every galaxy.
Characteristic rotation speed
Definition: A consistently defined velocity measure, often from the flat part or width of a rotation curve.
Why it matters here: It is the kinematic coordinate of the Tully-Fisher relation.
Relationship: Inclination-corrected spectral line width can serve as a proxy for \(v_c\).
Limitation or common confusion: Mixing velocity definitions changes the fitted slope and scatter.
Mass-to-light ratio
Definition: The ratio of inferred mass to emitted luminosity in a specified band.
Why it matters here: It links observed light to stellar mass and helps interpret scaling-relation residuals.
Relationship: Population synthesis predicts stellar mass-to-light ratio from age, metallicity, and IMF assumptions.
Limitation or common confusion: It is band-dependent and does not automatically include dark matter.
Intrinsic scatter
Definition: The astrophysical dispersion around a relation remaining after measurement errors are accounted for.
Why it matters here: It determines both the physical informativeness and distance precision of a scaling relation.
Relationship: Likelihood models separate observational uncertainty from a population-level scatter term.
Limitation or common confusion: Observed scatter is not all intrinsic if errors or selection are misspecified.
Inclination correction
Definition: The geometric conversion from projected line-of-sight rotation to the disk-plane speed.
Why it matters here: It is essential because a face-on disk shows little Doppler rotation even when rotating rapidly.
Relationship: For an ideal disk, observed amplitude scales approximately as \(v_c\sin i\).
Limitation or common confusion: Small inclination errors become severe near face-on orientation.