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

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Table 3:

The comparison between our results and those from previous papers.
Object	T₀₂ [K]	T₀₄ [K]	T₀₆ [K]	Source
HD 23 180		$48\pm37$		Sonnentrucker et al. (2007)^a
	$20 \pm 7$	$35\pm10$	$56\pm11$	this work
HD 147 889	$52\pm22$	$116\pm28$		Sonnentrucker et al. (2007)^b
	$40 \pm 16$	$60\pm 9$	$69\pm 5$	Kazmierczak et al. (2009)
HD 148 184		65		van Dishoeck & de Zeeuw (1984)
	$39\pm16$	$57\pm12$		Sonnentrucker et al. (2007)^b
	$40 \pm 40$	$62\pm21$	$67\pm10$	Kazmierczak et al. (2009)
HD 154 368		30		van Dishoeck & de Zeeuw (1984)
	$27\pm8$	$38\pm5$		Sonnentrucker et al. (2007)^b
	$24 \pm 11$	$38\pm10$	$52\pm 6$	this work
HD 169 454	$11\pm3$			Gredel & Munch (1986)
	15⁺¹⁰_-5			van Dishoeck & Black (1989)
	$24\pm6$	$37\pm5$		Sonnentrucker et al. (2007)^c
	$21 \pm 5$	$29\pm3$	$40\pm 3$	Kazmierczak et al. (2009)
HD 179 406		$57\pm11$		Sonnentrucker et al. (2007)^d
	$21 \pm 13$	$51\pm13$	$54\pm 7$	Kazmierczak et al. (2009)
HD 204 827	$35\pm 7$	$51 \pm 3$		Sonnentrucker et al. (2007)
	$34 \pm 34$	$42\pm 2$	$45\pm 2$	this work

^a, ^b, ^c, ^d Calculated by Sonnentrucker et al (2007) using the EWs of Hobbs (1981), van Dishoeck & de Zeeuw (1984), Gredel (1999) and Federman et al. (1994) respectively.

Source LaTeX | All tables | In the text

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