Millimeter-wave survey of molecular clouds around the W5-East triggered star-forming region

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Table 1:

Physical parameters at peak $T_{\rm a}^*$ position for each ¹³CO molecular cloud.
Cloud	l	b	$\alpha$	$\delta$	$T_{\rm a}^*$	$\delta v$ $^{{\rm 1}}$	$V_{\rm LSR}$ $^{{\rm 2}}$	r	$N({\rm H_2}$ )	Mass	BRC number
	(degree)	(degree)	(J2000.0)	(J2000.0)	(K)	(km s^-1)	(km s^-1)	(pc)	( $\times 10^{22}$ cm^-2)	( $M_{\odot}$ )
cloud 1	137.53	1.28	02 54 58	+60 36 06	9.4	1.55	-38.3	0.31	7.7	460	12
cloud 2	137.67	1.62	02 57 16	+60 50 20	6.09	1.93	-38.2	0.81	6.9	2 700	-
cloud 3	137.72	1.63	02 57 40	+60 49 28	4.66	1.41	-38.8	0.71	6.8	2 100	-
cloud 4	137.77	1.46	02 57 23	+60 39 02	16.3	1.46	-39.3	2.9	8.9	36 000	-
cloud 5	137.77	1.65	02 58 06	+60 49 08	7.58	1.17	-40.4	0.44	7.3	850	-
cloud 6	138.15	1.69	03 01 00	+60 40 29	11.6	1.66	-38.5	1.03	8.4	4 500	13
cloud 7	138.31	1.56	03 01 39	+60 29 02	15.1	2.27	-38.1	2.8	9.4	33 000	14
cloud 8	138.32	1.68	03 02 11	+60 35 05	7.65	1.38	-39.3	0.55	7.3	1 300	-

¹ FWHM of the Gaussian fit to the observed spectra.
² The velocity corresponding to the peak intensity of the Gaussian fit to the observed spectra.

Source LaTeX | All tables | In the text

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