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

Free Access

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

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.