Critical study of the distribution of rotational velocities of Be stars - I. Deconvolution methods, effects due to gravity darkening, macroturbulence, and binarity

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Volume 595 (November 2016)

A&A, 595 (2016) A132

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Table E.1

Test pnrc solutions parameters.


		Input apparent model-data					Solutions for pnrc parameters



η	i °	T _eff	log g		Vsini	Vsini	η	i °		log g_o		Vsini	V _c
		K			km s^-1	corr			K			corr	km s^-1


0.00	0°	20 000	4.00	3.461	0	0	0.00	0°	20 000	4.00	3.461	0	462


0.20	20°	19 665	3.95	3.496	81	81	0.20	20°	20 001	4.00	3.461	81	462
							0.22 ± 0.17	23° ± 10	20 093 ± 79	4.01 ± 0.02	3.462 ± 0.025	82 ± 6	465 ± 5
	50°	19 195	3.92	3.432	182	182	0.20	50°	20 002	4.00	3.461	182	462
							0.20 ± 0.13	48° ± 11	19 915 ± 79	3.99 ± 0.03	3.444 ± 0.018	184 ± 14	463 ± 5
	80°	18 758	3.88	3.372	234	234	0.20	80°	19 999	4.00	3.461	234	462
							0.22 ± 0.09	60° ± 10	19 792 ± 338	3.98 ± 0.03	3.424 ± 0.039	237 ± 18	462 ± 6


0.50	20°	19 555	3.90	3.572	119	122	0.46	22°	20 116	3.99	3.488	122	461
							0.45 ± 0.15	24° ± 6	20 114 ± 75	3.98 ± 0.02	3.496 ± 0.015	122 ± 9	460 ± 5
	50°	18 468	3.85	3.427	259	273	0.45	53°	20 092	4.00	3.476	270	462
							0.45 ± 0.09	54° ± 6	20 110 ± 224	4.00 ± 0.01	3.479 ± 0.017	271 ± 21	462 ± 5
	80°	17 209	3.74	3.259	334	351	0.51	71°	19 811	3.95	3.426	355	462
							0.54 ± 0.11	74° ± 8	20 051 ± 598	3.96 ± 0.02	3.448 ± 0.062	363 ± 36	466 ± 11


0.75	20°	19 143	3.89	3.615	126	143	0.75	20°	20 004	4.00	3.461	143	462
							0.73 ± 0.13	20° ± 2	19 965 ± 108	4.00 ± 0.00	3.457 ± 0.012	141 ± 11	462 ± 1
	50°	17 881	3.86	3.431	283	319	0.75	50°	20 000	4.00	3.460	320	462
							0.76 ± 0.11	50° ± 4	19 967 ± 262	4.00 ± 0.01	3.454 ± 0.026	317 ± 24	462 ± 4
	80°	16 214	3.76	3.189	346	411	0.75	80°	19 999	4.00	3.461	411	462
							0.76 ± 0.14	78° ± 7	19 758 ± 536	3.99 ± 0.02	3.434 ± 0.049	403 ± 42	459 ± 10

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