High-Resolution Spectroscopy of the Accretion Disk Corona source 4U 1822-37

Details High-Resolution Spectroscopy of the Accretion Disk Corona source 4U 1822-37 High-Resolution Spectroscopy of the Accretion Disk Corona source 4U 1822-37

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000head....5.2505c&link_type=abstract

American Astronomical Society, HEAD Meeting #5, #25.05; Bulletin of the American Astronomical Society, Vol. 32, p.1220

Astronomy and Astrophysics

Astronomy

Scientific paper

We present a preliminary analysis of the X-ray spectrum from the low-mass x-ray binary 4U 1822-37 that was obtained with the High Energy Transmission Grating Spectrometer (HETGS) onboard the Chandra Observatory. We discuss the plasma parameters derived from the observed spectral diagnostics and how these constrain models of accretion disk corona sources.

Affiliated with

Also associated with

No associations

Rating

High-Resolution Spectroscopy of the Accretion Disk Corona source 4U 1822-37 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with High-Resolution Spectroscopy of the Accretion Disk Corona source 4U 1822-37, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High-Resolution Spectroscopy of the Accretion Disk Corona source 4U 1822-37 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-871480