HRC-I/Chandra X-ray observations towards σ Orionis

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Table 3:

Sources with a probability of X-ray variability in the HRC-I data greater than $p_{\rm var}$ = 99.5 %.
No.	Name	$\overline{CR}$	$\chi ^2$	Variability
		[ks^-1]		type
4	Mayrit 348349	29.1	12.5	Flare decay
7	Mayrit 789281	54.9	24.8	Flare
8	Mayrit 863116 AB	55.6	26.3	Flare with structure
11	Mayrit 156353	13.0	3.6	Flare
13	Mayrit 180277	11.8	4.1	Flare
18	Mayrit 403090	11.0	4.5	Rot. modulation?
27	Mayrit 489165	8.0	3.2	Flare
28	Mayrit 489196	8.0	4.5	Rot. modulation?
30	Mayrit 397060	5.4	4.1	Flare

Source LaTeX | All tables | In the text

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