Comoving frame models of hot star winds - I. Test of the Sobolev approximation in the case of pure line transitions

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Volume 519 (September 2010)

A&A, 519 (2010) A50

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Table 1:

Radius R_*, mass M, and the effective temperature $T_{\rm eff}$ of studied model stars.
Star (model)		R_*	M	$T_{\rm eff}$
		$[R_\odot]$	$[M_\odot$ ]	[K]
First stars
M500-1		11.1	50	50 000
M500-2		33.7	50	29 900
M500-3		72.0	50	20 600
M500-4		303	50	10 100
O stars
$\xi$ Per	HD 24912	14.0	36	35 000
$\iota$ Ori	HD 37043	21.6	41	31 400
15 Mon	HD 47839	9.9	32	37 500
	HD 54662	11.9	38	38 600
	HD 93204	11.9	41	40 000
$\zeta$ Oph	HD 149757	8.9	21	32 000
68 Cyg	HD 203064	15.7	38	34 500
19 Cep	HD 209975	22.9	47	32 000
Central stars of planetary nebulae
NGC 2392		1.5	0.41	40 000
NGC 3242		0.3	0.53	75 000
IC 4637		0.8	0.87	55 000
IC 4593		2.2	1.11	40 000
He 2-108		2.7	1.33	39 000
IC 418		2.7	1.33	39 000
Tc 1		3.0	1.37	35 000
NGC 6826		2.2	1.40	44 000

Source LaTeX | All tables | In the text

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