The ISO Long Wavelength Spectrometer line spectrum of VY Canis Majoris and other oxygen-rich evolved stars

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Table 1:

Characteristics of the stars used in this paper.
Star name	Distance	Mass loss rate	Ref.
	(pc)	( $M_{\odot}$ yr^-1)
VY CMa	1100	0.5- $1 \times 10^{-4}$	(1), (2)
IK Tau	300	$4.9 \times 10^{-6}$	(3)
TX Cam	390	$2.6 \times10^{-6}$	(3)
RX Boo	160	$2.2 \times10^{-7}$	(4)
IRC+10011 (WX Psc)	830	$6 \times10^{-6}$	(5)
R Cas	107	$3.4 \times 10^{-7}$	(6)

Notes. (1) Reid & Menten (in preparation); Choi et al. (2008); (2) Decin et al. (2006); (3) Olivier et al. (2001); (4) Teyssier et al. (2006); (5) Decin et al. (2007); (6) Truong-Bach et al. (1999).

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