Bolometric luminosity variations in the luminous blue variable AFGL2298

J. S. Clark; P. A. Crowther; V. M. Larionov; I. A. Steele; B. W. Ritchie; A. A. Arkharov

doi:10.1051/0004-6361/200912358

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Volume 507 / No 3 (December I 2009)

A&A, 507 3 (2009) 1555-1565

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Table 5:

Summary of the total mass and nebular expansion velocity of LBV (top panel) and YHG (bottom panel) circumstellar ejecta.
Star	$v_{\rm neb}$	M	Reference
	(km s^-1)	( $M_{\odot}$ )
${\eta }$ Car (Homunculus)	650	>12	a
(Little Homunculus)	200	0.1	b
P Cygni	136	0.1	c
Pistol Star	60-95	11	d, e
AFGL 2298	70	10	f
AG Car	70	8.9	g, h
G79.29+0.46	44	15	i, j, k
Wra 751	26	1.7	g, l
HD 168625	19	2.1	m, n
IRC +10 420	27	0.24	o
	35	0.46	o
HD 179821	35	4.0	o

^a Smith et al. (2003); ^b Smith (2005); ^c Smith & Hartigan (2006); ^d Figer et al. (1999); ^e Figer et al. (1998); ^f Ueta et al. (2001); ^g Voors et al. (2000a); ^h Smith et al. (1991); ⁱ Higgs et al. (1994); ^j Waters et al. (1996); ^k Voors et al. (2000b); ^l Hutsemekers & van Drom (1991); ^m Pasquali et al. (2002); ⁿ O'Hara et al. (2003); ^o Castro-Carrizo et al. (2007).

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