Polar bulges and polar nuclear discs: the case of NGC 4698
E. M. Corsini (1, 2), J. M\'endez-Abreu (3, 4), N. Pastorello (1, and 5), E. Dalla Bont\`a (1, 2), L. Morelli (1, 2), A. Beifiori (6), A., Pizzella (1, 2), and F. Bertola (1, 2) ((1) Dipartimento di Fisica e, Astronomia, Universit\`a di Padova

TL;DR
This study reveals the complex, orthogonal structures of NGC 4698, showing a perpendicular bulge and nuclear disc likely formed through external gas acquisition and star formation over billions of years.
Contribution
It provides a detailed photometric analysis of NGC 4698's unique orthogonal bulge and nuclear disc, supporting a formation scenario involving external gas accretion.
Findings
Bulge elongated perpendicular to the main disc.
Nuclear disc is thin, exponential, and orientation-independent.
Star formation in the nuclear disc occurred over 5 Gyr ago.
Abstract
The early-type spiral NGC 4698 is known to host a nuclear disc of gas and stars which is rotating perpendicularly with respect to the galaxy main disc. In addition, the bulge and main disc are characterised by a remarkable geometrical decoupling. Indeed they appear elongated orthogonally to each other. In this work the complex structure of the galaxy is investigated by a detailed photometric decomposition of optical and near-infrared images. The intrinsic shape of the bulge was constrained from its apparent ellipticity, its twist angle with respect to the major axis of the main disc, and the inclination of the main disc. The bulge is actually elongated perpendicular to the main disc and it is equally likely to be triaxial or axisymmetric. The central surface brightness, scalelength, inclination, and position angle of the nuclear disc were derived by assuming it is infinitesimally thin…
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