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Although he does not use the term "amorphous" to describe these galaxies, it is the best description of these galaxies. The "wind effects" refer to the appearance, not the actual detection of high-velocity gas (such as is found in The long filaments in these systems are probably tidal tails or bridges that have been produced as the result of the gravitational interaction between the galaxies.
This category contains a mixture of different types of objects. This category contains a mix of interacting galaxies distorted by tidal interactions, nearby dwarf irregular galaxies, and spiral galaxies with unusual large amounts of gas.
Based on the description of these objects, it appears that Arp originally thought that the elliptical galaxies were pushing away spiral arms in companion galaxies. A peculiar galaxy is a galaxy of unusual size, shape, or composition. The "amorphous spiral arms" are the tidal debris that remains after the collision. Yet, there are many types of galaxies in the universe and they're not all spirals. If such a merger is relatively gentle and the galaxies are oriented properly with respect to each other, the final object will most likely resemble a spiral galaxy of some type. Such an object would have all the characteristics of what Hubble classified as an elliptical galaxy. The word "galaxy" brings to mind images of the Milky Way or perhaps the Andromeda galaxy, with their spiral arms and central bulges.These spiral galaxies are what people commonly imagine all galaxies look like.
Energy exchange will randomize stellar orbits, but stellar collisions would be rare, because stars are so small compared to their average separations. Finally, objects that simply do not fit into any of the above categories are listed as objects 332–338. Like the galaxies with diffuse filaments or galaxies with counter-tails, some of the galaxies in this category have been involved in interactions, and the filaments are tidal features created by those interactions. Such gas still emits radio radiation and may be observed in large blobs (the radio astronomers call these lobes) on either side of a galaxy. Strong shock fronts will develop and, contrary to the normal inefficiency of conversion of interstellar material into stars, there can be complete conversion of the gas into stars. The ejecta in many of these objects appear to be tidal features created by gravitational interactions. Two of the objects are connected by tidal bridges. Peculiar galaxy ESO 162-17, also known as LEDA 20531 or 2MASX J07155452-5720363, is a peculiar galaxy - a galaxy that has gone through interactions with its cosmic neighbors, resulting in an unusual amount of dust and gas, an irregular shape, or a strange composition. Peculiar Galaxies ENCYCLOPEDIA OF ASTRONOMY AND STROPHYSICS Peculiar Galaxies A peculiar galaxy is an object that cannot be easily classified as a SPIRAL, ELLIPTICAL,orIRREGULAR GALAXY based on its optical morphology. In some cases (such as for Almost all of the objects in this category are interacting or have recently undergone interactions. Objects 102–145 are elliptical and elliptical-like galaxies. The momentary compression of the interstellar gas, however, triggers major star formation and the appearance of a Gravitational interaction that disturbs the mass distribution in a galaxy may also trigger major events of nearly simultaneous star formation over the whole disk of a galaxy. The "jets" themselves look similar to water spraying out of a hose. At higher energy levels are hot jets of material streaming out of galactic nuclei at nearly the speed of light (a so‐called relativistic velocity as the rules of the theory of special relativity must be used to describe phenomena at these exceedingly high velocities). Spiral galaxies with low surface brightness companionsSpiral galaxies with small high surface brightness companionsSpiral galaxies with large high surface brightness companionsElliptical galaxies close to and perturbing spiral galaxiesGalaxies with irregularities, absorption, and resolutionSpiral galaxies with low surface brightness companionsSpiral galaxies with small high surface brightness companionsSpiral galaxies with large high surface brightness companionsElliptical galaxies close to and perturbing spiral galaxiesGalaxies with irregularities, absorption, and resolution The interaction process will produce various tidal features, such as tidal tails and tidal bridges, that may last well after the progenitor galaxies' disks and nuclei have merged. A total of 338 galaxies are presented in the atlas, which was originally published in 1966 by the California Institute of Technology. Although the tidal tails are described as several different visual phenomena ("counter-tails", "filaments", "loops"), they are all manifestations of the same phenomena. Astronomers have identified two types of peculiar galaxies: interacting galaxies and active galactic nuclei. As the small galaxy passes through the disk, its extra contribution to gravitation pulls in stars and interstellar material from the outer disk of the large galaxy. This is another category in which the majority of objects are interacting galaxies. These are galaxies with shell-like structures. Galaxies in this category have either irregular structures (irregularities), notable dust lanes (absorption), or a grainy appearance (resolution). Some spiral arm segments may appear detached because dust lanes in the spiral arms obscure the arms' starlight. Galaxies in this category are almost always clearly interacting sources.
Although he does not use the term "amorphous" to describe these galaxies, it is the best description of these galaxies. The "wind effects" refer to the appearance, not the actual detection of high-velocity gas (such as is found in The long filaments in these systems are probably tidal tails or bridges that have been produced as the result of the gravitational interaction between the galaxies.
This category contains a mixture of different types of objects. This category contains a mix of interacting galaxies distorted by tidal interactions, nearby dwarf irregular galaxies, and spiral galaxies with unusual large amounts of gas.
Based on the description of these objects, it appears that Arp originally thought that the elliptical galaxies were pushing away spiral arms in companion galaxies. A peculiar galaxy is a galaxy of unusual size, shape, or composition. The "amorphous spiral arms" are the tidal debris that remains after the collision. Yet, there are many types of galaxies in the universe and they're not all spirals. If such a merger is relatively gentle and the galaxies are oriented properly with respect to each other, the final object will most likely resemble a spiral galaxy of some type. Such an object would have all the characteristics of what Hubble classified as an elliptical galaxy. The word "galaxy" brings to mind images of the Milky Way or perhaps the Andromeda galaxy, with their spiral arms and central bulges.These spiral galaxies are what people commonly imagine all galaxies look like.
Energy exchange will randomize stellar orbits, but stellar collisions would be rare, because stars are so small compared to their average separations. Finally, objects that simply do not fit into any of the above categories are listed as objects 332–338. Like the galaxies with diffuse filaments or galaxies with counter-tails, some of the galaxies in this category have been involved in interactions, and the filaments are tidal features created by those interactions. Such gas still emits radio radiation and may be observed in large blobs (the radio astronomers call these lobes) on either side of a galaxy. Strong shock fronts will develop and, contrary to the normal inefficiency of conversion of interstellar material into stars, there can be complete conversion of the gas into stars. The ejecta in many of these objects appear to be tidal features created by gravitational interactions. Two of the objects are connected by tidal bridges. Peculiar galaxy ESO 162-17, also known as LEDA 20531 or 2MASX J07155452-5720363, is a peculiar galaxy - a galaxy that has gone through interactions with its cosmic neighbors, resulting in an unusual amount of dust and gas, an irregular shape, or a strange composition. Peculiar Galaxies ENCYCLOPEDIA OF ASTRONOMY AND STROPHYSICS Peculiar Galaxies A peculiar galaxy is an object that cannot be easily classified as a SPIRAL, ELLIPTICAL,orIRREGULAR GALAXY based on its optical morphology. In some cases (such as for Almost all of the objects in this category are interacting or have recently undergone interactions. Objects 102–145 are elliptical and elliptical-like galaxies. The momentary compression of the interstellar gas, however, triggers major star formation and the appearance of a Gravitational interaction that disturbs the mass distribution in a galaxy may also trigger major events of nearly simultaneous star formation over the whole disk of a galaxy. The "jets" themselves look similar to water spraying out of a hose. At higher energy levels are hot jets of material streaming out of galactic nuclei at nearly the speed of light (a so‐called relativistic velocity as the rules of the theory of special relativity must be used to describe phenomena at these exceedingly high velocities). Spiral galaxies with low surface brightness companionsSpiral galaxies with small high surface brightness companionsSpiral galaxies with large high surface brightness companionsElliptical galaxies close to and perturbing spiral galaxiesGalaxies with irregularities, absorption, and resolutionSpiral galaxies with low surface brightness companionsSpiral galaxies with small high surface brightness companionsSpiral galaxies with large high surface brightness companionsElliptical galaxies close to and perturbing spiral galaxiesGalaxies with irregularities, absorption, and resolution The interaction process will produce various tidal features, such as tidal tails and tidal bridges, that may last well after the progenitor galaxies' disks and nuclei have merged. A total of 338 galaxies are presented in the atlas, which was originally published in 1966 by the California Institute of Technology. Although the tidal tails are described as several different visual phenomena ("counter-tails", "filaments", "loops"), they are all manifestations of the same phenomena. Astronomers have identified two types of peculiar galaxies: interacting galaxies and active galactic nuclei. As the small galaxy passes through the disk, its extra contribution to gravitation pulls in stars and interstellar material from the outer disk of the large galaxy. This is another category in which the majority of objects are interacting galaxies. These are galaxies with shell-like structures. Galaxies in this category have either irregular structures (irregularities), notable dust lanes (absorption), or a grainy appearance (resolution). Some spiral arm segments may appear detached because dust lanes in the spiral arms obscure the arms' starlight. Galaxies in this category are almost always clearly interacting sources.