The turbulent life of NGC 4696 as told by its globular cluster system

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Volume 689 (September 2024)

A&A, 689 (2024) A342

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Table 3.

Properties of the five galaxies for which the models of the surface brightness distribution were calculated.

Name	RA	Dec	Type	v_hel	d	n
	(J2000)	(J2000)	(RC3)	(km s⁻¹)	(Mpc)
WISEA J124839.70–411605.1	$12^{h} 48^{m} 39 \overset{s}{.} 69$ $12^{\mathrm{h}}48^{\mathrm{m}}39{{\overset{\text{ s}}{.}}}69$	$- 41 ° 16' 05 \overset{″}{.} 60$ $-41\circ16{\prime}05{{\overset{\prime\prime}{.}}}60$	dE	2851.03	46.21 ± 3.26	6 − 8 − 10
WISEA J124831.02–411823.2	$12^{h} 48^{m} 31 \overset{s}{.} 03$ $12^{\mathrm{h}}48^{\mathrm{m}}31{{\overset{\text{ s}}{.}}}03$	$- 41 ° 18' 23 \overset{″}{.} 19$ $-41\circ18{\prime}23{{\overset{\prime\prime}{.}}}19$	dE	3003.02	48.46 ± 3.41	6 − 8 − 10
WISEA J124902.02–411533.7	$12^{h} 49^{m} 02 \overset{s}{.} 00$ $12^{\mathrm{h}}49^{\mathrm{m}}02{{\overset{\text{ s}}{.}}}00$	$- 41 ° 15' 33 \overset{″}{.} 30$ $-41\circ15{\prime}33{{\overset{\prime\prime}{.}}}30$	dE	2074.86	34.76 ± 2.66	6
WISEA J124846.61–411539.4	$12^{h} 48^{m} 46 \overset{s}{.} 61$ $12^{\mathrm{h}}48^{\mathrm{m}}46{{\overset{\text{ s}}{.}}}61$	$- 41 ° 15' 39 \overset{″}{.} 50$ $-41\circ15{\prime}39{{\overset{\prime\prime}{.}}}50$	?	?	?	6 − 8 − 10
ESO 322- G 093	$12^{h} 49^{m} 04 \overset{s}{.} 12$ $12^{\mathrm{h}}49^{\mathrm{m}}04{{\overset{\text{ s}}{.}}}12$	$- 41 ° 20' 19 \overset{″}{.} 60$ $-41\circ20{\prime}19{{\overset{\prime\prime}{.}}}60$	Sc	3468.90	55.32 ± 3.89	6 − 8 − 10

Notes. The columns show the name of the galaxy, the coordinates (RA and Dec), the type, the heliocentric velocity, and the distance as reported in NED (https://ned.ipac.caltech.edu). The last column show the numbers of the higher order harmonics used in ISOFIT to calculate the models of the surface brightness distribution, which were equal for the three filters.

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