Table 1: Class transitions of GRS 1915+105 reported in this paper.
FIGURE Satellite Date Orbit No. Class transition

Time (UT) obs. ID

1. IXAE 22th June, 1997 1, 3, 5 $\kappa$ $\rightarrow$ $\rho$

12:12^a

2. IXAE 25th June, 1997 3, 4, 5 " $\chi$ '' $\rightarrow$ $\rho$

11:12^a

3. IXAE 08th June, 1999 2, 3 " $\chi$ '' $\rightarrow$ $\theta$

11:02^a

3. RXTE 08th June, 1999 40702-01-03-00 " $\chi$ '' $\rightarrow$ $\theta$

13:52

5. IXAE 25th June, 2000 2, 3 " $\rho$ '' $\rightarrow$ $\alpha$

14:07^b

^a Observation time at the begining of the first orbit;
^b Observation time at the begining of the second orbit.

**Table 1:** Class transitions of GRS 1915+105 reported in this paper.
FIGURE	Satellite	Date	Orbit No.	Class transition
		Time (UT)	obs. ID
1.	IXAE	22th June, 1997	1, 3, 5	$\kappa$ $\rightarrow$ $\rho$
		12:12^a
2.	IXAE	25th June, 1997	3, 4, 5	" $\chi$ '' $\rightarrow$ $\rho$
		11:12^a
3.	IXAE	08th June, 1999	2, 3	" $\chi$ '' $\rightarrow$ $\theta$
		11:02^a
3.	RXTE	08th June, 1999	40702-01-03-00	" $\chi$ '' $\rightarrow$ $\theta$
		13:52
5.	IXAE	25th June, 2000	2, 3	" $\rho$ '' $\rightarrow$ $\alpha$
		14:07^b

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observation of class transitions
	3 Possible nature of the accretion flow emerging from class transitions
	4 Concluding remarks
	References