Low mass X-ray binaries are two gravitationally bound stars where the secondary is a normal solar type like star and the primary a compact object, i.e. a black hole or neutron star. Matter is transferred from the secondary, thereby forming an accretion di

• Listing ID: 2103
• Project Leader: INSTITUTO DE ASTROFISICA DE CANARIAS
• Start date: 3/16/2009
• End Date: 3/15/2012
• Region: Canary Islands
• Programme: FP7-PEOPLE-ERG-2008