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Exploring the hot galactic halo using shadows of high latitude clouds
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Juda, M. |
| Copyright Year | 2001 |
| Description | The objective of this proposal was to measure variations in the 1/4 keV emission from the galactic halo, using ROSAT (x-ray astronomy satellite) Position Sensitive Proportional Counters (PSPC) observations toward known enhancements in the absorbing column density along the line-of-sight out of the Galaxy. Target directions were selected to have a low total hydrogen column density but to also show significant gradients in the amount of absorbing material, as traced by Infrared Astronomical Satellite (IRAS) 100 micron emission, on angular scales that would be contained within the PSPC field of view. In addition, we restricted the galactic latitude of the target directions to be greater than 60 degrees or less than -60 degrees in order to enable a cleaner separation of Galactic halo emission from that of the Galactic disk. The observations would also provide a measurement of the brightness of the emission from the Local Bubble. |
| File Size | 192520 |
| Page Count | 3 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_20020023448 |
| Archival Resource Key | ark:/13960/t6tx88q4w |
| Language | English |
| Publisher Date | 2001-12-01 |
| Access Restriction | Open |
| Subject Keyword | Astrophysics Rosat Mission Halos Milky Way Galaxy Variations Emission Proportional Counters Infrared Astronomy Infrared Astronomy Satellite 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 |