**Table 3:** Interstellar regions within ${\sim} 1\hbox{$.\!\!^\circ$ }5$ from the position of V838 Mon.
No.	l b	Name	$T^{\ast}_A$	$V_{\rm LSR}$	Notes	References
	( $\hbox{$^\circ$ }$ ) ( $\hbox{$^\circ$ }$ )		(K)	(km s^-1)
1	216.5 +0.5			47.	MC	MAB
2	216.5 +1.2			48.	MC	MAB
3	217.0 +0.9	FT 84		51.	MC	Av, DHT
4	217.2 +0.5		2.6	52.	MC	Av, WB, MAB
5	217.3 +0.0			27.	MC	MAB
6	217.4 -0.1	FT 87, BFS 57	18.9	26.	MC	Av, WB
7	217.4 +0.3	FT 88, BFS 58	3.7	50.	MC	Av, WB, MAB
8	217.6 -0.2	FT 89, BFS 59	10.4	26.	MC	Av, WB
9	217.6 +2.4		6.3	55.	MC	Av, WB
10	217.9 +0.9				RN	Ma
11	218.0 +0.2			23.	MC	MAB
12	218.1 -0.3	S 287, FT 91	18.2	26.-30.	HII, MC	Av, WB, MAB
13	218.7 +1.8	IC 466, S 288	6.3	57.	HII, MC	Av, WB

Notes: HII - HII region, MC - molecular cloud, RN - reflection nebula.
References: Av - Avedisova (2002), DHT - $V_{\rm LSR}$ estimated from original data of Dame et al. (2001), Ma - Magakian (2003), MAB - May et al. (1997), WB - Wouterloot & Brand (1989).

Source LaTeX | All tables | In the text

	1 Introduction
	2 The analysis of the photometric data
	3 Circumstellar and interstellar environment
	4 Discussion and summary
	References