X-ray bursters and the X-ray sources of the galactic bulge

Details X-ray bursters and the X-ray sources of the galactic bulge X-ray bursters and the X-ray sources of the galactic bulge

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980stin...8122989l&link_type=abstract

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Astronomy and Astrophysics

Astronomy

Galactic Bulge, Galactic Evolution, Galactic Radiation, Galactic Radio Waves, Stellar Evolution, X Ray Astronomy, X Ray Scattering, X Ray Sources, Planetary Evolution, Solar Radio Bursts, Stellar Mass Accretion

Scientific paper

Type 1 X-ray bursts, optical, infrared, and radio properties of the galactic bulge sources, are discussed. It was proven that these burst sources are neutron stars in low mass, close binary stellar systems. Several burst sources are found in globular clusters with high central densities. Optical type 1 X-ray bursts were observed from three sources. Type 2 X-ray bursts, observed from the Rapid Burster, are due to an accretion instability which converts gravitational potential energy into heat and radiation, which makes them of a fundamentally different nature from Type 1 bursts.

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