Probing the disc wind-jet connection in black hole transients II
Abstract
We propose six observations of one high inclination black hole low mass X-ray binary (LMXB) at different stages of its outburst. We will investigate the presence of X-ray narrow absorption/emission features in the XMM spectra, which are a signature of a disc wind, and their relation to the accreting regime. Such features, identified with ions like FeXXV and FeXXVI, have been observed in a number of LMXBs and give us information about the mass outflow rate and the launching mechanism of the wind. With simultaneous radio observations we will probe the jet power as a function of the wind properties and how the radio flux density correlates with the X-ray flux at different accretion regimes. We will also investigate the broadening mechanism of the FeK emission line detected up to now in several LMXBs.
- Publication:
-
XMM-Newton Proposal
- Pub Date:
- October 2013
- Bibcode:
- 2013xmm..prop..168D
- Keywords:
-
- White Dwarf Binaries;
- Neutron Star Binaries;
- Cataclysmic Variables;
- ULXs;
- Black Holes;
- GRO J1655-40;
- GRO J1655-40;
- GRO J1655-40;
- GRO J1655-40;
- GRS 1009-45;
- GRS 1009-45;
- GRS 1009-45;
- GRS 1009-45;
- XTE J1550-564;
- XTE J1550-564;
- XTE J1550-564;
- XTE J1550-564;
- MAXI J1305-704;
- MAXI J1305-704;
- MAXI J1305-704;
- MAXI J1305-704;
- XTE J1650-50;
- XTE J1650-50;
- XTE J1650-50;
- XTE J1650-50;
- H 1705-250;
- H 1705-250;
- H 1705-250;
- H 1705-250;
- H 1743-322;
- H 1743-322;
- H 1743-322;
- H 1743-322;
- 4U 1755-33;
- 4U 1755-33;
- 4U 1755-33;
- 4U 1755-33;
- V 4641 Sgr;
- V 4641 Sgr;
- V 4641 Sgr;
- V 4641 Sgr;
- GS 2000+25;
- GS 2000+25;
- GS 2000+25;
- GS 2000+25;
- XTE J1118+48;
- XTE J1118+48;
- XTE J1118+48;
- XTE J1118+48;
- GS 2023+338;
- GS 2023+338;
- GS 2023+338;
- GS 2023+338;
- MAXI J1659-152;
- MAXI J1659-152;
- MAXI J1659-152;
- MAXI J1659-152;
- SWIFT J1357.2-0;
- SWIFT J1357.2-0;
- SWIFT J1357.2-0;
- SWIFT J1357.2-0;
- New BH transien;
- New BH transien;
- New BH transien;
- New BH transien