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The Milky Way's Central Molecular Zone

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arxiv 1705.05332 v1 pith:QUKKC5WM submitted 2017-05-15 astro-ph.GA

classification astro-ph.GA
keywords molecularcentercentralgalacticgalaxyregionreviewstudies
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This review compiles the results of recent studies of molecular gas conditions in the central six hundred parsecs of our Galaxy. The review begins by placing our Galactic center into context with the rest of our galaxy. It next discusses the wealth of previous research on the Galactic center, before focusing on what is known about the molecular interstellar medium in this region. It focuses especially on a surge in interest in this region and new studies conducted in the last five years. It concludes by highlighting open questions that remain, and the potential for new facilities such as ALMA to make progress in resolving these uncertainties.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. 25 years of XMM-Newton observations of the Sgr A complex: 3D distribution and internal structure of the clouds

    astro-ph.GA 2025-01 conditional novelty 6.0 of 10

    A 25-year X-ray light-echo study places the Sgr A molecular complex about 25 pc behind the Milky Way's central black hole and finds a roughly log-normal density distribution with a high-density excess.

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