... The nature of Coma's X-ray emission is still being investigated . Tomorrow's picture: Gas Clouds and Star Clusters . < Archive | Index | Search | ...
... Also known as Abell 426 , the center of the Perseus Cluster is a prodigious source of X-ray radiation , and so helps astronomers explore how clusters formed and how gas and dark matter interact . ...
... Also known as Abell 426, the center of the Perseus Cluster is a prodigious source of X-ray radiation , and so helps astronomers explore how clusters formed and how gas and dark matter interact. ...
... This cluster is loaded with gas and dust rich, star forming, spiral galaxies but has relatively few elliptical galaxies , which lack gas and dust and the associated newborn stars . ...
... Also known as Abell 426, the center of Perseus cluster is a prodigious source of X-ray radiation , and so helps us study how clusters formed and how gas and dark matter interact. ...
... Also known as Abell 426, the center of Perseus cluster is a prodigious source of X-ray radiation , and so helps astronomers study how clusters formed and how gas and dark matter interact. ...
... The hot wind of particles that streams away from the cluster stars contributes to an already complex menagerie of gas and dust filaments while slowly evacuating the cluster center. ...
... The hot wind of particles that streams away from the cluster stars contributes to an already complex menagerie of gas and dust filaments while slowly evacuating the cluster center. ...