Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...246l..17g&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 246, no. 1, June 1991, p. L17-L20.
Astronomy and Astrophysics
Astronomy
111
Accretion Disks, Black Body Radiation, Magellanic Clouds, X Ray Binaries, Photons, Point Sources, Rosat Mission, Satellite Observation, Spaceborne Astronomy
Scientific paper
The results of Rosat observations are given for CAL 83 and the new soft source RX J0527.8-6954 in the Large Magellanic Cloud (LMC). Both sources have remarkably similar spectra which can be described by black-body radiation. The best fit values of N(H) = (1-2) x 10 to the 21st/sq cm clearly indicate LMC membership for both sources. The sources exhibit black-body temperatures of 20-40 eV and radiate at the Eddington limit or even beyond. These sources may represent a new class of bright low-mass X-ray binaries which could help to solve the millisecond-pulsar birthrate problem.
Greiner Jochen
Hasinger Guenter
Kahabka Peter
No associations
LandOfFree
ROSAT observation of two supersoft sources in the Large Magellanic Cloud 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 ROSAT observation of two supersoft sources in the Large Magellanic Cloud, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and ROSAT observation of two supersoft sources in the Large Magellanic Cloud will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1277811