On the genesis of spiral galaxies -- Classical and pseudo bulges as extremities of a continuous sequence
Iris Breda, Polychronis Papaderos

TL;DR
This study analyzes star formation histories of 135 late-type galaxies, revealing a continuous spectrum of bulge and disk properties that supports a unified inside-out formation process rather than two distinct formation routes.
Contribution
It provides evidence that classical and pseudo bulges are part of a continuous sequence, challenging the idea of two separate formation mechanisms for LTG bulges.
Findings
Bulge and disk properties show a continuous distribution across galaxy mass.
Higher mass LTGs exhibit shorter formation timescales.
No bimodal correlations support a unified formation scenario.
Abstract
A tantalizing enigma in extragalactic astronomy concerns the chronology and driving mechanisms of the build-up of late-type galaxies (LTGs). The standard scenario envisages two formation routes, with classical bulges (CBs) assembling first in a quick quasi-monolithic episode followed by gradual disk assembly, and pseudo-bulges (PBs) forming over the Gyr-long secular evolution of LTGs. The expectation is, therefore, the segregation of present-day LTG bulges into two distinct groups. Here we analyse the star formation histories (SFHs) of bulges and disks for 135 LTGs from the CALIFA survey covering the relevant range in LTG mass. In addition, their physical properties were contrasted with predictions from evolutionary synthesis models, adopting exponentially declining SFHs, with an e-folding time 0.1 < < 20 Gyr. Analysis of the SFHs of ~ half-million spaxels consistently reveals…
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