X-ray lines from accreting black holes

Details X-ray lines from accreting black holes X-ray lines from accreting black holes

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974a%26a....35..171m&link_type=abstract

Astronomy and Astrophysics, vol. 35, no. 2, Oct. 1974, p. 171-176.

Astronomy and Astrophysics

Astronomy

14

Astronomical Models, Black Holes (Astronomy), Emission Spectra, Line Spectra, X Ray Astronomy, Angular Velocity, Deposition, Doppler Effect, Forbidden Transitions, Gravitational Effects, Magnetohydrodynamic Stability, Radiative Transfer, Resonance Scattering, Scattering Cross Sections, Spectral Line Width

Scientific paper

The X-ray emission line spectrum of black holes surrounded by accretion disks is considered. For steady-state disks, we calculate the expected line strengths, equivalent widths and broadening. This is done for the L-alpha line of S(15+), using a representative set of disk parameters, and for the intercombination and forbidden lines of Fe(24+), for a range of disk parameter. The values predicted differ from those of other models of X-ray sources, and are such that experimental detection appears feasible.

Affiliated with

Also associated with

No associations

Rating

X-ray lines from accreting black holes 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 X-ray lines from accreting black holes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and X-ray lines from accreting black holes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-791187