X-ray temperatures and their radial distributions from winds of O-type supergiants: the effects of clumps

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Table 1:

Line widths of the program stars.
	Ion	Theoretical	Observational
$\zeta$ Ori A	O VII	610-880	500^a, $900\pm200$ ^b
	Ne IX	610-880	1360^a, $900\pm200$ ^b
	Mg XI	480-800	$900\pm200$ ^b
	Si XIII	360-700	$900\pm200$ ^b
$\zeta$ Pup	O VII	900-1100
	Ne IX	780-1050
	Mg XI	690-990
	Si XIII	350-700

Notes. ^(a) Cohen et al. (2006); ^(b) Waldron & Cassinelli (2000); ^(c) Kahn et al. (2001).

Source LaTeX | All tables | In the text

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