Molecular gas and star formation in the Milky Way
Francoise Combes (LERMA, Obs-Paris)
TL;DR
This paper reviews the role of dense molecular gas as a tracer of the Milky Way's spiral structure, discusses current simulation models of gas flows, and suggests improvements incorporating star formation insights from external galaxies.
Contribution
It provides a comprehensive summary of current gas flow simulations in the Milky Way and proposes enhancements by integrating star formation processes based on external galaxy studies.
Findings
Molecular gas effectively traces the Milky Way's spiral structure.
Current simulations can be improved by including star formation physics.
External galaxy studies offer valuable insights for modeling the Milky Way.
Abstract
The dense molecular gas is the ideal tracer of the spiral structure in the Milky Way, and should be used intensively to solve the puzzle of its structure. In spite of our position inside the plane, we can hope to disentangle the structures, with position-velocity diagrams, in addition to . I summarize the state of the art simulations of gas flows in the MW, and describe what can be done to improve the models, taking into account the star formation, in view of what is already done in external galaxies, with a more favorable viewing angle.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.