Molecular tendrils feeding star formation in the Eye of the Medusa - The Medusa merger in high resolution 12CO 2–1 maps

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Volume 569 (September 2014)

A&A, 569 (2014) A6

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Table 1

Properties of the identified GMA candidates.

GMA	RA(2000)	Dec(2000)	Spherical radius^a	v₀^b	Dispersion^c	Mass
	[h] [m] [s]	[°] [′] [′′]	[pc]	[km s^-1]	[km s^-1]	[M_⊙]

GMA 1	12:14:09.805	54:31:35.54	83	2585	42	1.0 × 10⁷
GMA 2	12:14:09.749	54:31:36.01	103	2501	52	1.5 × 10⁷
GMA 3	12:14:09.631	54:31:36.08	92	2467	44	1.2 × 10⁷
GMA 4	12:14:09.737	54:31:35.47	132	2557	57	3.4 × 10⁷
GMA 5	12:14:09.674	54:31:35.76	114	2508	67	2.8 × 10⁷
GMA 6	12:14:09.632	54:31:35.44	92	2510	62	1.6 × 10⁷
GMA 7	12:14:09.749	54:31:34.72	123	2595	40	3.1 × 10⁷
GMA 8	12:14:09.667	54:31:35.13	130	2595	45	3.5 × 10⁷
GMA 9	12:14:09.612	54:31:33.90	103	2599	45	1.9 × 10⁷
GMA 10	12:14:09.577	54:31:34.21	130	2575	59	3.1 × 10⁷
GMA 11	12:14:09.547	54:31:34.55	92	2588	47	1.3 × 10⁷

Notes.

^(a)

The source size was determined by fitting a Gaussian to the position of the respective GMA in the uv table. The values given here are the FWHM of the fitted Gaussian deconvolved from the synthesized beam. The typical (average) error for the fit to the GMA size is about 20%.

^(b)

Typical errors are on the order of 5−10 km s^-1.

^(c)

Typical errors are on the order of 10%.

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