Abstract: Humans have recognized the natural entity of galaxies for over ninety years. Dr.He initiated the concept of rational structure and applied it to the study of galaxy struc-ture in 2001. The main reason is that galaxy arms trace their way on the galaxy disk plane elegantly so that the ratio of stellar density on the left side of the route to the one on the right is constant along the way. This is comparable to the elegant principle of natural selec-tion. From now on, we call galaxy arms ‘Darwin spirals ’ or ‘Darwin curves ’ instead of calling them ‘iso-ratio curves ’ or ‘proportion curves’. If Dr.He’s study is proved to be truth, then galaxy arms must be the disturbance to rational structure. The disturbance generates dus
In this paper, we study the morphological properties of spiral galaxies, including measurements of s...
In this paper, we study the morphological properties of spiral galaxies, including measurements of s...
The onset of spiral structure in galaxies appears to occur between redshifts 1.4 and 1.8 when disks ...
Abstract Weakly interacted galaxies present very simple body structure. They are either three-dimens...
Abstract Rational structure in two dimension means that not only there exists an orthogonal net of c...
Abstract Weakly interacted galaxies present very simple body structure. They are either three-dimens...
We use classifications provided by citizen scientists though Galaxy Zoo to investigate the correlati...
Using an equation of motion for a self-gravitating filament, we show how galactic spiral arms might ...
Context. Spiral galaxies are very common in the local Universe, but their formation, evolution, and ...
Abstract Context.: Spiral galaxies are very common in the local Universe, but their formation, evol...
We present here the results of an imaging study of eight grand-design and two intermediate-arm galax...
We describe a system that builds quantitative structural descriptions of spiral galaxies. This enabl...
In this paper we study the morphological properties of spiral galaxies, including measurements of sp...
Spiral structure is the most distinctive feature of disk galaxies and yet debate persists about whic...
Spiral structure is the most distinctive feature of disk galaxies and yet debate persists about whic...
In this paper, we study the morphological properties of spiral galaxies, including measurements of s...
In this paper, we study the morphological properties of spiral galaxies, including measurements of s...
The onset of spiral structure in galaxies appears to occur between redshifts 1.4 and 1.8 when disks ...
Abstract Weakly interacted galaxies present very simple body structure. They are either three-dimens...
Abstract Rational structure in two dimension means that not only there exists an orthogonal net of c...
Abstract Weakly interacted galaxies present very simple body structure. They are either three-dimens...
We use classifications provided by citizen scientists though Galaxy Zoo to investigate the correlati...
Using an equation of motion for a self-gravitating filament, we show how galactic spiral arms might ...
Context. Spiral galaxies are very common in the local Universe, but their formation, evolution, and ...
Abstract Context.: Spiral galaxies are very common in the local Universe, but their formation, evol...
We present here the results of an imaging study of eight grand-design and two intermediate-arm galax...
We describe a system that builds quantitative structural descriptions of spiral galaxies. This enabl...
In this paper we study the morphological properties of spiral galaxies, including measurements of sp...
Spiral structure is the most distinctive feature of disk galaxies and yet debate persists about whic...
Spiral structure is the most distinctive feature of disk galaxies and yet debate persists about whic...
In this paper, we study the morphological properties of spiral galaxies, including measurements of s...
In this paper, we study the morphological properties of spiral galaxies, including measurements of s...
The onset of spiral structure in galaxies appears to occur between redshifts 1.4 and 1.8 when disks ...