Modelling of dust around the symbiotic Mira RR Telescopii during obscuration epochs

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Table 9

Luminosities and temperatures of the hot and cool components of RR Tel and HM Sge.

Parameter	RR Tel	HM Sge

L_cool (L_⊙)	7350¹–9450²	5000³–10 600⁴
T_hot (K)	140 000^5,⁶	100 000–200 000^3,^4,⁶
L_hot (L_⊙)	3500⁵–9000⁶	9000^3,⁴

Notes.

⁽¹⁾

PL relation of Whitelock et al. (1994).

⁽²⁾

PL relation of Guandalini & Busso (2008).

⁽³⁾

Schild et al. (2001).

⁽⁴⁾

Bogdanov & Tarranova (2001).

⁽⁵⁾

Nussbaumer & Dumm (1997), Jordan et al. (1994).

⁽⁶⁾

Muerset et al. (1991).

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