Excitation temperature of and broadening of the 6196 Å diffuse interstellar band

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Table 2:

Summary of observational data
Object	FWHM(6196)[Å]	T₀₂(C₂)^a[K]	T₀₄(C₂)^a[K]	T₀₆(C₂)^a[K]	FWHM(CH 4300)[Å]
HD 23 180 ¹	$0.41\pm 0.06$	$20 \pm 7$	$35\pm10$	$56\pm11$	$0.095\pm0.019$
HD 110 432²	$0.38\pm 0.07$	$13 \pm 4$	$27\pm 6$		$0.120\pm0.014$
HD 147 888³	$0.51\pm 0.07$	$38 \pm 20$	$66\pm13$		$0.101\pm0.013$
HD 147 889⁴	$0.52\pm 0.02$	$40 \pm 16$	$60\pm 4$	$69\pm 5$	$0.079\pm0.005$
HD 148 184⁴	$0.55\pm 0.02$	$40 \pm 40$	$62\pm21$	$67\pm10$	$0.067\pm0.007$
HD 149 757⁵	$0.49\pm 0.05$	$36 \pm 12$	$74\pm15$		$0.058\pm0.006$
HD 154 368¹	$0.42\pm 0.03$	$24 \pm 11$	$38\pm10$	$52\pm 6$	$0.076\pm0.006$
HD 163 800⁴	$0.39\pm 0.02$	$25 \pm 8$	$66\pm21$	$56\pm 8$	$0.066\pm0.006$
HD 169 454⁴	$0.42\pm 0.03$	$21 \pm 5$	$29\pm3$	$40\pm 3$	$0.082\pm0.007$
HD 179 406⁴	$0.34\pm 0.02$	$21 \pm 13$	$51\pm13$	$54\pm 7$	$0.081\pm0.005$
HD 204 827⁶	$0.38\pm 0.05$	$34 \pm 34$	$42\pm 2$	$45\pm 2$	$0.146\pm0.015$

FWHM(6196) and FWHM(CH 4300) were measured in this paper.
^a For ¹ Were measured in this paper.
^a For ² Were calculated by Sonnentrucker et al. (2007) using the EW's of van Dishoeck & Black (1989).
^a For ³ - Sonnentrucker et al (2007).
^a For ⁴ - Kazmierczak et al. (2009).
^a For ⁵ Were calculated by Sonnentrucker et al. (2007) using the EW's of Hobbs & Campbell (1982).
^a For ⁶ Were calculated in this work based on EW's from Ádámkovics et al. (2003).

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