Two generations in stellar complexes and associations in M 33 galaxy and their spatial correlation
Todor Veltchev, Nina Koleva, Petko Nedialkov, G. R. Ivanov
TL;DR
This study analyzes the massive stellar populations in M 33's stellar complexes and associations using multi-band photometry to understand their formation and spatial distribution.
Contribution
It introduces a combined photometric approach to distinguish stellar populations and reconstruct star formation history in M 33.
Findings
Identification of OB stars and red supergiants in M 33
Insights into the spatial correlation of stellar populations
Reconstruction of star formation processes in the galaxy
Abstract
Massive stellar content of stellar complexes and associations in M 33 is studied combining deep UBV photometry from the Local Group Survey (Massey et al. 2006) and JHK photometry from the 2MASS. Two basic populations (incl. OB stars and red supergiants) are distinguished and their application for reconstruction of the star formation process in this galaxy are discussed.
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.
Taxonomy
TopicsAstronomy and Astrophysical Research · Galaxies: Formation, Evolution, Phenomena · Stellar, planetary, and galactic studies