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- W1633425311 abstract "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." @default.
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- W1633425311 date "2001-12-01" @default.
- W1633425311 modified "2023-10-16" @default.
- W1633425311 title "Exploring the Hot Galactic Halo Using Shadows of High Latitude Clouds" @default.
- W1633425311 hasPublicationYear "2001" @default.
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