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Gas-based time projection chambers (TPCs) have been shown to be highly sensitive X-ray polarimeters having excellent quantum efficiency while at the same time achieving large modulation factors. To ob...
We present the first observations of emission lines of CN(2-1), HCO$^{+}$(3-2) and C$_{2}$H(3-2) in the Perseus cluster. We observed at two positions: directly at the central galaxy, NGC 1275 and also...
Gas Heating, Chemistry, and Infrared Spectra in Intermediate-Aged Disks Around Low Mass Stars。
The X-ray irradiated gas around a compact object was investigated. Wesolved the hydrostatic balance coupling with the ionization and thermal balancesto obtain the structure of the optically thin emiss...
Hot gas and the gaseous structure of the galaxy     HYDRODYNAMICS  SUPERNOVAREMNANTS  X-RAYS  GALAXIES       font style='font-size:12px;'> 2009/6/4
A parochial review is presented concerning the status of our understandingof hot gas regions in the Galaxy and their implications for the overall distributionsof the Galaxy抯 gaseous components. We hav...
Hot gas in the galaxy:what do we know for sure?      GENERAL GALAXY  BUBBLES ISM  GENERAL X-RAYS       font style='font-size:12px;'> 2009/6/4
Major advances have been made in the past decade in our knowledge of the hotinterstellar gas of our Milky Way galaxy. The Di.use X-ray Spectrometer obtainedspectra in the 0.15?.28 keV range from the G...

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