REVIEW 1 cited by
The Milky Way's Central Molecular Zone
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
read the original abstract
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.
Forward citations
Cited by 1 Pith paper
-
25 years of XMM-Newton observations of the Sgr A complex: 3D distribution and internal structure of the clouds
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.
Discussion (0). Continue with ORCID to comment.