3 edition of X-ray spectral and temporal studies of the ultra-compact system X1916-05 found in the catalog.
X-ray spectral and temporal studies of the ultra-compact system X1916-05
Jonathan E. Grindlay
Published
1998 by National Aeronautics and Space Administration, National Technical Information Service, distributor in [Washington, DC, Springfield, Va .
Written in English
Edition Notes
| Statement | submitted by Jonathan E. Grindlay, principal investigator. |
| Series | [NASA contractor report] -- NASA/CR-208208., NASA contractor report -- NASA CR-208208. |
| Contributions | United States. National Aeronautics and Space Administration. |
| The Physical Object | |
|---|---|
| Format | Microform |
| Pagination | 1 v. |
| ID Numbers | |
| Open Library | OL15507822M |
An empirical method of determining momentary discharge of tide-affected streams
Legalism.
Contracts and agreements for public library service.
defence industry environment and its impact on the military-industrial firm.
potential applications of desktop publishing in information services
Drawings of the old masters in the University galleries and in the Library of Christ church, Oxford
Wildlife Services program
Investigations into the feasibility of an on-line test methodology
Ross Poldark
breakdown of democratic regimes : Chile
Analytical Coordination Chemistry Section
historical review of Coventry Cathedral and its potential as an educational resource
Norman Parkinson
Thailand at a glance
Get this from a library. X-ray spectral and temporal studies of the ultra-compact system X final report (8/15//14/98), grant NAG [Jonathan E Grindlay; United States. National Aeronautics and Space Administration.]. Buy X-ray spectral and temporal studies of the ultra-compact system X final report (8/15/96 - 2/14/98), grant NAG (SuDoc NAS ) by Jonathan E.
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The extremely populous GC system of NGC has an extent of at least kpc, which is comparable to the core radius of the Fornax cluster itself.
Here, the mass estimates obtained from the combined analysis of the GCs and the stellar velocity dispersion profile agree with the values from X-ray studies in the inner kpc.
At larger radii.
