Spectral characteristics of 3U 1915-05, a burst source candidate

Details Spectral characteristics of 3U 1915-05, a burst source candidate Spectral characteristics of 3U 1915-05, a burst source candidate

Sep 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...216l.101b&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 216, Sept. 15, 1977, p. L101-L104.

Astronomy and Astrophysics

Astronomy

27

Bursts, Light Curve, Spaceborne Astronomy, X Ray Sources, X Ray Spectra, Astronomical Models, Oso-8, Thermal Radiation

Scientific paper

An X-ray burst source has been discovered near the X-ray source 3U 1915-05. The continuum spectra of both the burst source and the quiescent source 3U 1915-05 are hard, with kT for thermal bremsstrahlung models above 20 keV. The spectrum of 3U 1915-05 has a feature at 9.1 keV, which, if attributed to absorption by hydrogen and heliumlike iron, suggests the presence of a highly ionized cloud surrounding a central X-ray source.

Affiliated with

Also associated with

No associations

Rating

Spectral characteristics of 3U 1915-05, a burst source candidate 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 Spectral characteristics of 3U 1915-05, a burst source candidate, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectral characteristics of 3U 1915-05, a burst source candidate will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1093295