MAGNUM survey: Compact jets causing large turmoil in galaxies - Enhanced line widths perpendicular to radio jets as tracers of jet-ISM interaction

G. Venturi; G. Cresci; A. Marconi; M. Mingozzi; E. Nardini; S. Carniani; F. Mannucci; A. Marasco; R. Maiolino; M. Perna; E. Treister; J. Bland-Hawthorn; J. Gallimore

doi:10.1051/0004-6361/202039869

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Volume 648 (April 2021)

A&A, 648 (2021) A17

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Table 2.

Basic information about the four galaxies presented.

Name	Distance	FOV extent	Spatial scale
	[Mpc] ^(a)	[kpc²] ^(b)	[pc arcsec⁻¹] ^(c)
IC 5063	46 ± 7	14 × 14	220
NGC 5643	16 ± 7	5 × 5	78
NGC 1068	10.5 ± 1.7	3.3 × 3.3	51
NGC 1386	16.4 ± 0.8	5.1 × 5.1	80

Notes.

^(a)

Distance of the galaxy from Earth, obtained from http://leda.univ-lyon1.fr/ best distance modulus, i.e. the weighted average between the redshift distance modulus corrected for infall of the Local Group towards Virgo and the weighted average of the published redshift-independent distance measurements.

^(b)

Central portion of the galaxy covered by the MUSE ∼1′×1′ FOV.

^(c)

Spatial scale at the distance of the galaxy.

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