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Table 2.

Parameters characterizing the scenarios.

Parameter Symbol (a) Value Comments
– General –
Distance to the tip of the object L 60 kpc Fig. 1
Width of the object 2r 2 kpc Fig. 1
Stellar mass of the 2nd galaxy 7 × 109M Fig. 1; vD23
Stellar mass of the object 3 × 109M Fig. 1; vD23
Redshift of the object 1 vD23
Tolerance in the TFR Δlog Vmax 0.1 dex Sánchez Almeida et al. (2023)
Present age of the Universe tH 13.5 Gyr
– Runaway SMBH –
Star formation efficiency 1 Gyr−1 Leroy et al. (2008)
Age of the stellar trail 39 Myr vD23
Gas mass needed to form the object Mg 7.7 × 1010M Sect. 2.2
Sound speed cs 10 km s−1 Sect. 2.2
Temperature of the gas 104 K Sect. 2.2
Jeans length λJ 5 × 10−2 kpc Sect. 2.2
Free fall time in the halo of the host tfila 150 Myr Sect. 2.2
Number of big filaments per galaxy nfila 2 Sect. 2.2
Mass of the SMBH M 7 × 106M Sect. 2.3; vD23
Velocity of the SMBH v 1600 km s−1 vD23
Width of the wake 2d 2 kpc Fig. 2, with d = r
Distance SMBH to gas clouds dmin 1 kpc dmin = r; Eq. (9)
Density of the gas ρ 7 × 10−25 g cm−3 Sects. 2.2 and 2.3
Bondi–Hoyle–Lyttleton accretion radius Racc 2.3 × 10−2 pc Eq. (10)
Galaxies without stellar trail Nno 1.5 × 106 SDSS, Ahn et al. (2012)
Thermal velocity of the gas vther ∼7 km s−1 Sect. 2.4
Scape velocity from the 2nd galaxy vesc ∼400 km s−1 Sect. 2.4
– Bulgeless edge-on galaxy –
Radius of the edge-on disk Ra 25 kpc Figs. 1 and 3
Full width of the edge-on disk Wa 2 kpc Wa = 2r; Sect. 3
Number surface density of galaxies Σg > 1 Mpc−2 Sect. 3
Full width of the 2nd galaxy Wb 6 kpc Wb = 3Wa; Fig. 3b

Notes.

(a)

Empty boxes correspond to parameters without specific symbols in the main text.

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