A method to determine distances to molecular clouds using near-IR photometry

G. Maheswar; C. W. Lee; H. C. Bhatt; S. V. Mallik; S. Dib

doi:10.1051/0004-6361/200912594

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Volume 509 (January 2010)

A&A, 509 (2010) A44

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Table 2:

Distances to the clouds L1517, Cha I, Lup 3 and NGC 7023 compiled from the literature.
Cloud	Distances quoted	Associated	Ref.
Identification	in the literature (pc)	star
L 1517	$\rm 144^{+23}_{-17}$ $^{\dag }$	AB Aur	1
Chamaeleon 1	115-215, 158	HD 97048	2, 3
	$150\pm15$ , $\rm 175^{+27}_{-20}$		4, 1
Lupus 3	130-170, 140	HR 5999	5, 6, 7
	100, $\rm 208^{+46}_{-32}$ , $140\pm2$		8, 9, 10
NGC 7023	440, $\rm 429^{+159}_{-90}$ , $288\pm25$	HD 200775	11, 1
	$288\pm25$		12

1-Bertout et al. (1999); 2-Schwartz (1991); 3-Franco (1991); 4-Whittet et al. (1997); 5-Murphy et al. (1986); 6-Krautter (1991); 7-Hughes et al. (1993); 8-Knude & Høg (1998); 9-van den Ancker et al. (1998); 10-de Zeeuw et al. (1999); 11-Viotti (1969); 12-Straizys et al. (1992).
$^{\dag }$ The Hipparcos distance to the AB Aur.

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