Young stars and reflection nebulae near the lower “edge” of the Galactic molecular disc

P. M. Palmeirim; J. L. Yun

doi:10.1051/0004-6361/200913224

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Volume 510 (February 2010)

A&A, 510 (2010) A51

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Table 1:

Photometry of the optical nebula stars.
ID	Multiplicity	RA	Dec	m_V	$m_{K\!_{\rm S}}$	$(H-K_{\rm S})$	$(J-K_{\rm S})$
		(2000)	(2000)
A	$\ldots$	07 40 14.7	-33 32 34	14.90	12.46	0.24	0.65
B^a	1	07 40 15.8	- 33 32 39	15.27	13.04	0.29	0.95
	2	07 40 15.8	- 33 32 40	15.27	12.36	0.26	0.76
C	$\ldots$	07 40 16.1	- 33 32 31	15.20	13.66	0.16	0.45

Notes. ^(a) This star is double, as revealed by our near-IR images. The V-band magnitude quoted here corresponds to the combined flux of both stars, unresolved in the optical image.

Source LaTeX | All tables | In the text

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