Two Pseudobulges in the "Boxy Bulge" Galaxy NGC 5746

TL;DR

This study identifies a distinct, secularly-evolved pseudobulge within galaxy NGC 5746, challenging traditional galaxy formation models by showing a pure-disk galaxy lacking a classical bulge.

Contribution

It provides observational evidence of a secondary pseudobulge in NGC 5746, separate from the boxy bulge, highlighting secular evolution in a galaxy expected to have a classical bulge.

Findings

Inner pseudobulge has Sersic index n < 2.

Pseudobulge contributes about 13.6% of total galaxy light.

Galaxy shows no signs of merger-built bulge, indicating secular evolution.

Abstract

Galaxy formation and growth under the {\Lambda}CDM paradigm is expected to proceed in a hierarchical, bottom-up fashion by which small galaxies grow into large galaxies; this mechanism leaves behind large "classical bulges" kinematically distinct from "pseudobulges" grown by internal, secular processes. We use archival data (Spitzer 3.6 \mum wavelength, Hubble Space Telescope H-band, Two Micron All Sky Survey Ks-band, and Sloan Digital Sky Survey gri-band) to measure composite minor- and major-axis surface brightness profiles of the almost-edgeon spiral galaxy NGC 5746. These light profiles span a large range of radii and surface brightnesses to reveal an inner, high surface brightness stellar component that is distinct from the well-known boxy bulge. It is well fitted by S\'ersic functions with indices n = 0.99 \pm 0.08 and 1.17 \pm 0.24 along the minor and major axes, respectively. Since n < 2, we conclude that this innermost component is a secularly-evolved pseudobulge that is distinct from the boxy pseudobulge. This inner pseduobulge makes up 0.136 \pm 0.019 of the total light of the galaxy. It is therefore considerably less luminous than the boxy structure, which is now understood to be a bar seen nearly end-on. The infrared imagery shows further evidence for secular evolution in the form of a bright inner ring of inner radius 9.1 kpc and width 1.6 kpc. NGC 5746 is therefore a giant, pure-disk SB(r)bc galaxy with no sign of a merger-built bulge. We do not understand how such galaxies form in a {\Lambda}CDM universe.