The source GRS 1915+105 was observed in March 6-7 as part of a
on-going monitoring campaign (PI: Hannikainen). GRS 1915+105 is
one of the galactic sources which shows jets (sometimes called a
'micro-quasar') and is a Black Hole Candidate. The source is
known for its remarkable time variability. An example of the time
variability is shown here. The data has been obtained with JEM-X,
the X-ray instrument on-board INTEGRAL. GRS 1915+105 is currently
undergoing an outburst and will be observed again on April 2 as
part of the INTEGRAL core program.
Courtesy: Diana Hannikainen, Osmi Vilhu, Soren Brand and the JEM-X team
