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Main Authors: Zoccali, Manuela, Valenti, Elena
Format: Preprint
Published: 2024
Subjects:
Online Access:https://arxiv.org/abs/2412.01607
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author Zoccali, Manuela
Valenti, Elena
author_facet Zoccali, Manuela
Valenti, Elena
contents This chapter reviews the three-dimensional structure, age, kinematics, and chemistry of the Milky Way (MW) region within ~2 kpc from its center (hereafter referred to as the 'bulge') from an observational perspective. While not exhaustive in citations, this review provides historical context and discusses the main controversies and limitations in the current consensus. The nuclear bulge region, within $\sim$200 pc from the Galactic center, has been excluded from this review. This very complex region, hosting dense molecular clouds and active star formation, would deserve a dedicated paper.
format Preprint
id arxiv_https___arxiv_org_abs_2412_01607
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle The Milky Way Bulge
Zoccali, Manuela
Valenti, Elena
Astrophysics of Galaxies
This chapter reviews the three-dimensional structure, age, kinematics, and chemistry of the Milky Way (MW) region within ~2 kpc from its center (hereafter referred to as the 'bulge') from an observational perspective. While not exhaustive in citations, this review provides historical context and discusses the main controversies and limitations in the current consensus. The nuclear bulge region, within $\sim$200 pc from the Galactic center, has been excluded from this review. This very complex region, hosting dense molecular clouds and active star formation, would deserve a dedicated paper.
title The Milky Way Bulge
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2412.01607