We analyzed the 2003 Target of Opportunity XMM-Newton observation of IGR J16318-4848, to derive the properties of the matter responsible for the obscuration and for the emission of Fe and Ni lines. The line of sight material has a column density of about 2 x 10(24) cm(-2) but, from the Fe K alpha line EW and Compton Shoulder, we argue that the average column density is a few x 10(23) cm(-2), while the covering factor is about 0.1-0.2. The iron K alpha line varies on time scales as short as 1000 s, implying a size of the emitting region less than 3 x 10(13) cm. An ongoing XMM-Newton/INTEGRAL monitoring campaign is confirming the non-transient nature of the source.
Matt, G., Guainazzi, M. (2005). The properties of the absorbing and line emitting material in IGR J16318-4848. CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS, 5, 99-103.
The properties of the absorbing and line emitting material in IGR J16318-4848
MATT, Giorgio;
2005-01-01
Abstract
We analyzed the 2003 Target of Opportunity XMM-Newton observation of IGR J16318-4848, to derive the properties of the matter responsible for the obscuration and for the emission of Fe and Ni lines. The line of sight material has a column density of about 2 x 10(24) cm(-2) but, from the Fe K alpha line EW and Compton Shoulder, we argue that the average column density is a few x 10(23) cm(-2), while the covering factor is about 0.1-0.2. The iron K alpha line varies on time scales as short as 1000 s, implying a size of the emitting region less than 3 x 10(13) cm. An ongoing XMM-Newton/INTEGRAL monitoring campaign is confirming the non-transient nature of the source.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
