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KINEMATICS OF DIFFUSE ELLIPTICAL GALAXIES.

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Title: KINEMATICS OF DIFFUSE ELLIPTICAL GALAXIES.
Authors: Prugniel, PH.1 prugniel@obs.univ-lyon1.fr, Simien, F.1
Source: Astrophysics & Space Science. 2003, Vol. 284 Issue 2, p603-606. 4p.
Subjects: Elliptical galaxies, Galactic dynamics, Astronomy, Astrophysics, Space sciences, Physics
Abstract: New observations show that most of the flattened diffuse elliptical (dE) galaxies are essentially isotropic rotators. This supports the idea that dEs have evolved from fast rotating dIrr systems or late-type spirals after their gas was expelled by SN-driven winds and stripped by ram pressure against the intergalactic medium. [ABSTRACT FROM AUTHOR]
Copyright of Astrophysics & Space Science is the property of Springer Nature and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
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  Data: KINEMATICS OF DIFFUSE ELLIPTICAL GALAXIES.
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  Data: <searchLink fieldCode="DE" term="%22Elliptical+galaxies%22">Elliptical galaxies</searchLink><br /><searchLink fieldCode="DE" term="%22Galactic+dynamics%22">Galactic dynamics</searchLink><br /><searchLink fieldCode="DE" term="%22Astronomy%22">Astronomy</searchLink><br /><searchLink fieldCode="DE" term="%22Astrophysics%22">Astrophysics</searchLink><br /><searchLink fieldCode="DE" term="%22Space+sciences%22">Space sciences</searchLink><br /><searchLink fieldCode="DE" term="%22Physics%22">Physics</searchLink>
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  Data: New observations show that most of the flattened diffuse elliptical (dE) galaxies are essentially isotropic rotators. This supports the idea that dEs have evolved from fast rotating dIrr systems or late-type spirals after their gas was expelled by SN-driven winds and stripped by ram pressure against the intergalactic medium. [ABSTRACT FROM AUTHOR]
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  Data: <i>Copyright of Astrophysics & Space Science is the property of Springer Nature and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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        Value: 10.1023/A:1024014207820
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      – SubjectFull: Galactic dynamics
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      – SubjectFull: Astronomy
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      – TitleFull: KINEMATICS OF DIFFUSE ELLIPTICAL GALAXIES.
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