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Studies of gas in cooling flow clusters
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Cowie, Lennox L. Hu, Esther M. |
| Copyright Year | 1991 |
| Description | This report describes studies of cooling flows in rich clusters of galaxies, found to be sources of strong, extended X-ray emission seen by the EINSTEIN satellite. Two complementary lines of investigation were pursued: (1) studies of the dust content of the cluster gas using multi-wavelength data from archival records of the IUE and IRAS satellites in combination with previously obtained optical, and (2) coronal line spectroscopic studies of the bright emission systems. |
| File Size | 96529 |
| Page Count | 3 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19940008486 |
| Archival Resource Key | ark:/13960/t7fr4sm5v |
| Language | English |
| Publisher Date | 1991-10-31 |
| Access Restriction | Open |
| Subject Keyword | Fluid Mechanics And Heat Transfer Satellite Observation Astronomical Spectroscopy Infrared Astronomy Satellite Stellar Coronas Galactic Clusters Light Emission Cosmic Dust Interstellar Extinction Emission Spectra Iue X Ray Spectra Cooling Flows Astrophysics Line Spectra X Ray Sources Ntrs Nasa Technical Reports ServerĀ (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Technical Report |