We present the preliminary analysis of a 10 ks XMM-Newton EPIC/pn observation of Cir X-1 immediately after the zero phase. The continuum emission is modeled using a blackbody component partially absorbed by neutral matter probably located around the binary system. We detect a forest of emission lines associated to highly ionized ions
Aims:We present the results of the analysis of an archival observation of LMC X-2 performed with XMM...
We present new optical and infrared (IR) observations of Cir X-1 taken near apastron. Both sets of s...
Context. The properties of the X-ray emission lines are a fundamental tool for studying the nature o...
We present the preliminary analysis of a 10 ks XMM-Newton EPIC/pn observation of Cir X-1 immediately...
We present the results of a 54 ks long Chandra observation of the peculiar source Cir X-1. We perfor...
We present the results of an archival 54 ks long Chandra observation of the peculiar source Cir X-1 ...
Circinus X-1 (Cir X-1) is a neutron star binary with an elliptical orbit of 16.6~days. The source is...
IGR J16318-4848 is the prototype and one of the more extreme examples of the new class of highly obs...
We report on the results of a BeppoSAX (1.8--200 keV) observation of the peculiar X-ray binary sourc...
We present the preliminary spectral analysis of a 25 ks long Chandra observation of the peculiar sou...
We present X-ray spectra of the nucleus of the nearby radio galaxy Centaurus A from observations wit...
We report on a 300 ks BeppoSAX(0.12-200 keV) observation of Circinus X-1 (CirX-1) at phases between ...
We report on a 70 ks XMM-Newton Target of Opportunity (ToO) observation of the newly discovered accr...
We present new optical and infrared (IR) observations of Cir X-1 taken near apastron. Both sets of s...
Context. Circinus X-1 is a neutron-star-accreting X-ray binary in a wide (Porb = 16.6 d), eccentric ...
Aims:We present the results of the analysis of an archival observation of LMC X-2 performed with XMM...
We present new optical and infrared (IR) observations of Cir X-1 taken near apastron. Both sets of s...
Context. The properties of the X-ray emission lines are a fundamental tool for studying the nature o...
We present the preliminary analysis of a 10 ks XMM-Newton EPIC/pn observation of Cir X-1 immediately...
We present the results of a 54 ks long Chandra observation of the peculiar source Cir X-1. We perfor...
We present the results of an archival 54 ks long Chandra observation of the peculiar source Cir X-1 ...
Circinus X-1 (Cir X-1) is a neutron star binary with an elliptical orbit of 16.6~days. The source is...
IGR J16318-4848 is the prototype and one of the more extreme examples of the new class of highly obs...
We report on the results of a BeppoSAX (1.8--200 keV) observation of the peculiar X-ray binary sourc...
We present the preliminary spectral analysis of a 25 ks long Chandra observation of the peculiar sou...
We present X-ray spectra of the nucleus of the nearby radio galaxy Centaurus A from observations wit...
We report on a 300 ks BeppoSAX(0.12-200 keV) observation of Circinus X-1 (CirX-1) at phases between ...
We report on a 70 ks XMM-Newton Target of Opportunity (ToO) observation of the newly discovered accr...
We present new optical and infrared (IR) observations of Cir X-1 taken near apastron. Both sets of s...
Context. Circinus X-1 is a neutron-star-accreting X-ray binary in a wide (Porb = 16.6 d), eccentric ...
Aims:We present the results of the analysis of an archival observation of LMC X-2 performed with XMM...
We present new optical and infrared (IR) observations of Cir X-1 taken near apastron. Both sets of s...
Context. The properties of the X-ray emission lines are a fundamental tool for studying the nature o...