Accretion onto LLAGNs is still poorly understood. In this work we focus on the LINER galaxy M81, for which several different physical models (from standard accretion disks to advection dominated flows) have been invoked to explain its X-ray spectrum. The long (132 ks) XMM-Newton/pn observation of M81 has been analysed to test all the models proposed in literature
International audienceWe study the contribution of thermal and non-thermal processes to the inverse ...
A Chandra ACIS-S imaging observation of the nearby galaxy M81 (NGC 3031) reveals nine luminous soft ...
We report on a 63-ks long XMM-Newton observation of the accreting millisecond pulsar SAX J1808.4-365...
Accretion onto LLAGNs is still poorly understood. In this work we focus on the LINER galaxy M81, for...
We present the soft X-ray spectrum of the LINER galaxy M81 from a long observation with the XMM-Newt...
We present the soft X-ray spectrum of the LINER galaxy M 81 derived from a long observation with the...
We present the results of simultaneous Suzaku and NuSTAR observations of the nearest low-luminosity ...
Our group has used the High Energy Transmission Gratings (HETG) on board the Chandra X-ray telescope...
We present Chandra HETGS observations of the low-luminosity active galactic nucleus (LLAGN) of M81. ...
Despite advances in our understanding of low-luminosity active galactic nuclei (LLAGNs), the fundame...
We present results from the analysis of deep ROSAT HRI and PSPC observations of the spiral galaxy M8...
A new model is presented which explains the origin of the broad emission lines observed in the LINER...
The results of a spectral analysis, using {\it XMM-Newton} and {\it Chandra} data of the brightest u...
We report on a 63-ks long XMM-Newton observation of the accreting millisecond pulsar SAX J1808.4-365...
We report performance verification observations of the giant elliptical galaxy M87 in the Virgo Clus...
International audienceWe study the contribution of thermal and non-thermal processes to the inverse ...
A Chandra ACIS-S imaging observation of the nearby galaxy M81 (NGC 3031) reveals nine luminous soft ...
We report on a 63-ks long XMM-Newton observation of the accreting millisecond pulsar SAX J1808.4-365...
Accretion onto LLAGNs is still poorly understood. In this work we focus on the LINER galaxy M81, for...
We present the soft X-ray spectrum of the LINER galaxy M81 from a long observation with the XMM-Newt...
We present the soft X-ray spectrum of the LINER galaxy M 81 derived from a long observation with the...
We present the results of simultaneous Suzaku and NuSTAR observations of the nearest low-luminosity ...
Our group has used the High Energy Transmission Gratings (HETG) on board the Chandra X-ray telescope...
We present Chandra HETGS observations of the low-luminosity active galactic nucleus (LLAGN) of M81. ...
Despite advances in our understanding of low-luminosity active galactic nuclei (LLAGNs), the fundame...
We present results from the analysis of deep ROSAT HRI and PSPC observations of the spiral galaxy M8...
A new model is presented which explains the origin of the broad emission lines observed in the LINER...
The results of a spectral analysis, using {\it XMM-Newton} and {\it Chandra} data of the brightest u...
We report on a 63-ks long XMM-Newton observation of the accreting millisecond pulsar SAX J1808.4-365...
We report performance verification observations of the giant elliptical galaxy M87 in the Virgo Clus...
International audienceWe study the contribution of thermal and non-thermal processes to the inverse ...
A Chandra ACIS-S imaging observation of the nearby galaxy M81 (NGC 3031) reveals nine luminous soft ...
We report on a 63-ks long XMM-Newton observation of the accreting millisecond pulsar SAX J1808.4-365...