Non-circular motions and the cusp-core discrepancy in dwarf galaxies

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Table 2:

The main observational parameters.
Galaxy	Telescope	Arrays	Spectral resolution	Synthesised beam		Noise	References
			[ $\ensuremath{\mbox{km}~\mbox{s}^{-1}}$ ]	$^{\prime\prime}$ $\times$ $^{\prime\prime}$	pc $\times$ pc	mJy beam^-1
NGC 2366	VLA	B+C+D	2.6	$13 \times 12$	$217 \times 200$	0.5	(1)
ESO059-G001	ATCA	EW352+750C+1.5B	4	$51 \times 47$	$1130 \times 1041$	1.3	(2)
ESO215-G?009	ATCA	EW352+750A+1.5C+6A	4	$21 \times 21$	$530 \times 530$	1.0	(2)
NGC 4861	VLA	C+D	5.2	$31 \times 30$	$1127 \times 1091$	0.6	(3)
NGC 5408	ATCA	375+750D+1.5A	4	$57 \times 50$	$1329 \times 1166$	1.9	(4)
IC 5152	ATCA	EW367+750A+1.5A	4	$50 \times 43$	$502 \times 432$	1.5	(2)

References: (1) Walter et al. (2008); (2) Koribalski et al. (2009); (3) van Eymeren et al. (2009b); (4) van Eymeren (2008).

Source LaTeX | All tables | In the text

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