Lifetime of merger features of equal-mass disk mergers

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Volume 566 (June 2014)

A&A, 566 (2014) A97

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Table 2

Initial orbital configurations.

Simulation^a	Pair^b	e^c	R_peri^d	i_host^e

SbSb0p	Sb-Sb	1	5	0
SbSb45p	Sb-Sb	1	5	45
SbSb90p	Sb-Sb	1	5	90
SbSb135p	Sb-Sb	1	5	135
SbSb180p	Sb-Sb	1	5	180
SaSb45p	Sa-Sb	1	5	45
SaSb90p	Sa-Sb	1	5	90
SaSb135p	Sa-Sb	1	5	135
SbSb45r	Sb-Sb	1	0	45
SbSb45p+	Sb-Sb	1	10	45
SbSb45e	Sb-Sb	0.95	5	45
SbSb45h	Sb-Sb	1.05	5	45
SbSb₃45h	Sb-Sb₃	1.05	5	45
SbSb₆45h	Sb-Sb₆	1.05	5	45
SbSb₁₀45h	Sb-Sb₁₀	1.05	5	45
SbSb45hC	Sb-Sb	0.95^f	472^f	−

Notes.

^(a)

Types of galaxies, initial encounter angle, orbital shape (“p” for parabolic, “r” for radial, “e” for elliptical, “h” for hyperbolic, and “+” for larger pericentric distance), and additional cluster potential (“C” for cluster potential) are marked in the simulation name.

^(b)

Host-companion pair.

^(c)

Eccentricity of orbit.

^(d)

Pericentric distance (kpc).

^(e)

Inclination of host galaxy (°).

^(f)

The orbital parameters with respect to a cluster potential.

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