Add to ORKGAlmost 60 percent of nearby galaxies are spiral galaxies,which show the most beautiful and striking spiral structure.Spiral galaxies have been studied for more 70 years,but we still don’t clear the physical conditionAlmost 60 percent of nearby galaxies are spiral galaxies,which show the most beautiful and striking spiral structure.Spiral galaxies have been studied for more 70 years,but we still don’t clear the physical condition中国天文学会
We use an automated galaxy morphology analysis method to quantitatively measure the spirality of gal...
Abstract Weakly interacted galaxies present very simple body structure. They are either three-dimens...
In this paper, we study the morphological properties of spiral galaxies, including measurements of s...
We describe a system that builds quantitative structural descriptions of spiral galaxies. This enabl...
This thesis describes a system that, given approximately-centered images of spiral galaxies, produce...
Context. Spiral galaxies are very common in the local Universe, but their formation, evolution, and ...
Context. The Sérsic profile is a widely used model for describing the surface brightness distributio...
Abstract Context.: Spiral galaxies are very common in the local Universe, but their formation, evol...
In this paper we study the morphological properties of spiral galaxies, including measurements of sp...
We present here the results of an imaging study of eight grand-design and two intermediate-arm galax...
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 Carnegie-Irvine Galaxy Survey provide high quality$BVRI$broadband images for detail study of spi...
International audienceWe investigate how the properties of spiral arms relate to other fundamental g...
Abstract. This paper presents some new statistical correlations between the properties of disks and ...
We use an automated galaxy morphology analysis method to quantitatively measure the spirality of gal...
Abstract Weakly interacted galaxies present very simple body structure. They are either three-dimens...
In this paper, we study the morphological properties of spiral galaxies, including measurements of s...
We describe a system that builds quantitative structural descriptions of spiral galaxies. This enabl...
This thesis describes a system that, given approximately-centered images of spiral galaxies, produce...
Context. Spiral galaxies are very common in the local Universe, but their formation, evolution, and ...
Context. The Sérsic profile is a widely used model for describing the surface brightness distributio...
Abstract Context.: Spiral galaxies are very common in the local Universe, but their formation, evol...
In this paper we study the morphological properties of spiral galaxies, including measurements of sp...
We present here the results of an imaging study of eight grand-design and two intermediate-arm galax...
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 Carnegie-Irvine Galaxy Survey provide high quality$BVRI$broadband images for detail study of spi...
International audienceWe investigate how the properties of spiral arms relate to other fundamental g...
Abstract. This paper presents some new statistical correlations between the properties of disks and ...
We use an automated galaxy morphology analysis method to quantitatively measure the spirality of gal...
Abstract Weakly interacted galaxies present very simple body structure. They are either three-dimens...
In this paper, we study the morphological properties of spiral galaxies, including measurements of s...