A New Formula Describing the Scaffold Structure of Spiral Galaxies

TL;DR

This paper introduces a new mathematical formula that effectively models various spiral galaxy structures, including bars and rings, and correlates well with galaxy classification types.

Contribution

The paper presents a novel analytic formula for spiral galaxy shapes that unifies different structures and provides a better correlation with Hubble galaxy types than traditional models.

Findings

The new formula accurately fits diverse spiral galaxy shapes.

The pitch parameter correlates strongly with Hubble classification.

The formula can describe both constant and variable pitch spirals.

Abstract

We describe a new formula capable of quantitatively characterizing the Hubble sequence of spiral galaxies including grand design and barred spirals. Special shapes such as ring galaxies with inward and outward arms are also described by the analytic continuation of the same formula. The formula is r(phi) = A/log[B tan(phi/2N)]. This function intrinsically generates a bar in a continuous, fixed relationship relative to an arm of arbitrary winding sweep. A is simply a scale parameter while B, together with N, determine the spiral pitch. Roughly, greater N results in tighter winding. Greater B results in greater arm sweep and smaller bar/bulge while smaller B fits larger bar/bulge with a sharper bar/arm junction. Thus B controls the "bar/bulge-to-arm" size, while N controls the tightness much like the Hubble scheme. The formula can be recast in a form dependent only on a unique point of turnover angle of pitch - essentially a 1-parameter fit, aside from a scale factor. The recast formula is remarkable and unique in that a single parameter can define a spiral shape with either constant or variable pitch capable of tightly fitting Hubble types from grand design spirals to late type large-barred galaxies. We compare the correlation of our pitch parameter to Hubble type with that of the traditional logarithmic spiral for 21 well-shaped galaxies. The pitch parameter of our formula produces a very tight correlation with ideal Hubble type suggesting it is a good discriminator compared to logarithmic pitch, which shows poor correlation here similar to previous works. Representative examples of fitted galaxies are shown.