VLTI/MIDI observations of 7 classical Be stars | Astronomy & Astrophysics (A&A)

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Table 3:

Published effective temperature for our target stars.
Reference	Method	Effect of	Effective temperature [K]
		rotation	$\kappa$ CMa	$\delta$ Cen	$\alpha$ Ara	p Car	$\zeta$ Tau	$\alpha$ Col	$\beta$ CMi
Dachs et al. (1988)	Spectro-Photometry	No	22 500	22 500	18 000	16 500	-	13 000	-
Dachs et al. (1990)	Balmer Decrement	No	22 500	20 000	18 000	22 500	-	-	-
Chauville et al. (2001)	Spectroscopy	No	21 330	21 527	19 010	17 906	20 137	13 031	-
Fremat et al. (2005)	Spectroscopy	Yes	24 627	22 360	18 044	17 389	19 310	12 963	11 772
Levenhagen & Leister (2006)	Spectroscopy	No	24 100	22 230	22 150	-	-	14 200	13 100

Source LaTeX | All tables | In the text

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