Searching for X-ray emission from AGB stars | Astronomy & Astrophysics (A&A)

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Table 1

AGB stars discussed in detail in the paper.

Source	Sp.	Var.	P¹	L²	D^a
	type	type	[d]	[L_⊙]	[pc]

UX Ara	···	M	250	4570	1000:
T Cas	M	M	445	9200	290³
TX Cam	M	M	557	11 900	440⁴
o Cet	M	M	332	6430	92⁵
W Cyg	M	SRb	131	···	173⁵
R Dor	M	SRb	338	···	55⁵
T Dra	C	M	422	6550	610⁶
RT Eri	M	M	371	7380	277⁷
R Leo	M	M	310	5920	71⁵
L₂ Pup	M	SRb	141	···	64⁵
RW Sco	M	M	388	7800	870:
R UMa	M	M	302	5750	415⁵
SS Vir	C	SRa	364	···	540⁶

Notes.

^(a)

When a reliable parallax (p/Δp > 2) is available, it has been used to estimate the distance. For the remaining objects we have estimated the distance using the K-band magnitude (Skrutskie et al. 2006) and PL relation (Whitelock et al. 2008) (marked by a colon).

References.

⁽¹⁾

Samus et al. (2009);

⁽²⁾

Whitelock et al. (1994); Groenewegen & Whitelock (1996);

⁽³⁾

Loup et al. (1993);

⁽⁴⁾

Ramstedt et al. (2008);

⁽⁵⁾

van Leeuwen (2007);

⁽⁶⁾

Schöier & Olofsson (2001);

⁽⁷⁾

Knapp et al. (2003).

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