Predicting HCN, HCO, multi-transition CO, and dust emission of star-forming galaxies - From local spiral and ultraluminous infrared galaxies to high-z star-forming and submillimeter galaxies

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Volume 602 (June 2017)

A&A, 602 (2017) A51

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Table B.3

Submillimeter galaxies.

Galaxy name	v _rot	l _flat	l _∗	M _∗ ^c		L _TIR		Q ^b	δ ^b	Ṁ ^a	M _gas ^a
	(km s^-1)	(kpc)	(kpc)	(10¹⁰M_⊙)	(M_⊙ yr^-1)	(10¹¹L_⊙)	(^d)			(M_⊙ yr^-1)	(10⁹M_⊙)

SMM J02399-013	590	0.10	3.5	10.0	2294	68.8	49.0	1.5	5.0	1927.0	318.5
SMM J09431+470	295	0.10	0.9	10.0	1746	52.4	25.0	1.5	5.0	1117.4	39.1
SMM J105141+57	457	0.10	2.1	10.0	1296	38.9	50.0	1.5	5.0	423.4	98.2
SMM J123549+62	442	0.10	0.6	24.0	1794	53.8	40.0	1.5	5.0	71.8	17.1
SMM J123634+62	343	0.10	2.8	10.0	930	27.9	34.0	1.5	5.0	737.8	117.0
SMM J123707+62	317	0.10	1.9	24.0	1016	30.5	19.0	1.5	5.0	135.5	45.6
SMM J131201+42	430	0.10	2.1	10.0	1340	40.2	30.0	1.5	5.0	589.6	99.5
SMM J131232+42	346	0.10	1.4	10.0	1016	30.5	28.0	1.5	5.0	257.4	41.5
SMM J163650+40	523	0.10	1.6	46.0	1772	53.2	69.0	1.5	5.0	59.1	50.8
SMM J163658+41	590	0.10	0.5	52.0	2248	67.4	56.0	1.5	5.0	28.5	16.0

Notes.

^(a)

Calculated quantities;

^(b)

assumed quantities; all other columns are input quantities from Genzel et al. (2010);

^(c)

we assumed M_∗ = 10¹¹M_⊙ for galaxies whose mass is not given in Genzel et al. (2010);

^(d)

in 10⁹ K km s^-1 pc².

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