Abstract
The SS433 system ejects two relativistic jets with a velocity of 0.26c. The two jets are in oppsite directions, precessing with a period of 160 days 1. The system is assumed to include a compact object which rotates around a normal star with a period of 13 days2,3. There are strong indications for the presence of an accretion disk around the compact object 4. Based on study of a photometric light curve obtained during 3 years of observations5, we suggest here that the compact object might be a black hole.
Original language | English |
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Pages (from-to) | 341-342 |
Number of pages | 2 |
Journal | Nature |
Volume | 307 |
Issue number | 5949 |
DOIs | |
State | Published - 1984 |