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 4:

Summary of the progenitor and peak bolometric luminosities of the extragalactic SNe imposters (top panel) and the dust enshrouded optical transients (lower panel).
Transient	$\log(L_{\ast}/L_{\odot})$		Reference
	progenitor	outburst
SN 1961V	6.4	8.7	a, b
SN 1954J	5.7	6.5	b
SN 1997bs	<6.2	7.4	c
SN 2000ch	6.2	6.9	d
NGC 300-OT1	4.5	6.6	e
	4.7	7.1	f
SN 2008S	4.5	7.5	g, h

Luminosities assume a bolometric correction of ${\sim}0$ as appropiate for an F supergiant. References are ^a Goodrich et al. (1989); ^b Humphreys et al. (1999); ^c Van Dyk et al. 2000); ^d Wagner et al. (2004); ^e Bond et al. (2009); ^f Berger et al. (2009); ^g Smith et al. (2009); ^h Prieto et al. (2008).

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