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The stellar host in star-forming low-mass galaxies: Evidence for two classes
- Publication Year :
- 2019
- Publisher :
- arXiv, 2019.
-
Abstract
- The morphological evolution of star-forming galaxies provides important clues to understand their physical properties, as well as the triggering and quenching mechanisms of star formation. We aim at connecting morphology and star-formation properties of low-mass galaxies (median stellar mass $\sim$ 10$^{8.5}$ M$_{\odot}$) at low redshift ($z<br />Comment: Accepted for publication in Astronomy & Astrophysics. 13 pages, 11 figures
- Subjects :
- Physics
Stellar mass
010308 nuclear & particles physics
Star formation
FOS: Physical sciences
Astronomy and Astrophysics
Astrophysics
Astrophysics::Cosmology and Extragalactic Astrophysics
Astrophysics - Astrophysics of Galaxies
01 natural sciences
Instability
Redshift
Galaxy
Space and Planetary Science
Astrophysics of Galaxies (astro-ph.GA)
0103 physical sciences
Spectral energy distribution
Astrophysics::Solar and Stellar Astrophysics
Surface brightness
Astrophysics::Earth and Planetary Astrophysics
Low Mass
010303 astronomy & astrophysics
Astrophysics::Galaxy Astrophysics
Subjects
Details
- Database :
- OpenAIRE
- Accession number :
- edsair.doi.dedup.....ecb2ebc47889c899fd7b3fb73404e238
- Full Text :
- https://doi.org/10.48550/arxiv.1904.10462