A song of interactions and mergers: The case of NGC 4709

Open Access

Table 3.

Properties of the models of the surface brightness distribution of NGC 4709 in the i′ band.

Name	x₀	y₀	PA	e	SMA₀	SMA_max	RA	Dec	r_eff
	(pixels)	(pixels)	(°)		(arcmin)	(arcmin)	(J2000)	(J2000)	(arcmin)
NGC 4709	4117.31	6923.66	−76.22	0.12	0.719	1.864	$12^{h} 50^{m} 03 \overset{s}{.} 97$ $12^{\mathrm{h}}50^{\mathrm{m}}03{{\overset{\text{s}}{.}}}97$	$- 41 ° 22' 54 \overset{″}{.} 83$ $-41^\circ22{\prime}54{{\overset{\prime\prime}{.}}}83$	0.166

Notes.

The columns show the name of the galaxy, the fixed parameters used to fit the external isophotes (x₀, y₀, PA, e), the values of the semi-major axis between which the isophotes were calculated with fixed parameters (SMA₀ and SMA_max), the coordinates of the center of NGC 4709 corresponding to x₀ and y₀ (RA and Dec), and the effective radius derived from the model (r_eff).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.