Letizia Scaloni

ORCID: 0009-0002-6167-6728
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About
Contact & Profiles
Research Areas
  • Stellar, planetary, and galactic studies
  • Astronomy and Astrophysical Research
  • Astrophysics and Star Formation Studies
  • Astronomical Observations and Instrumentation
  • Galaxies: Formation, Evolution, Phenomena

The main sequence (MS) of star-forming galaxies (SFGs) is the tight relation between galaxy stellar mass and its star formation rate (SFR) was observed up to z ~ 6. MS can be used as a reference for understanding differences among galaxies, characterised by different rates production (starbursts, SFGs, passive galaxies), those inside made components (bulge, disk, halo). To investigate peculiar features found in our sample we focus here on their history (SFH). We performed spectral energy...

10.48550/arxiv.2403.18156 preprint EN arXiv (Cornell University) 2024-03-26

Context. The main sequence (MS) of star-forming galaxies (SFGs) is the tight relation between galaxy stellar mass ( M ⋆ ) and its star formation rate (SFR) was observed up to z ∼ 6. MS can be used as a reference for understanding differences among galaxies, which are characterised by different rates production (starbursts, SFGs, passive galaxies), those inside that made components (bulge, disk, halo). To investigate peculiar features found in our sample more depth, we focus here on their...

10.1051/0004-6361/202347626 article EN cc-by Astronomy and Astrophysics 2024-04-02

Stellar bars are common morphological structures in the local Universe; according to optical and NIR surveys, they present about two-thirds of disc galaxies. These elongated also believed play a crucial role secular evolutionary processes, because able efficiently redistribute gas, stars, angular momentum within their hosts, although it remains unclear as whether enhance or suppress star formation. A useful tool investigate this ambiguity is main sequence (MS) relation, which tightly links...

10.1051/0004-6361/202449894 preprint EN arXiv (Cornell University) 2024-04-17

Context. Stellar bars are common morphological structures in the local Universe; according to optical and NIR surveys, they present about two-thirds of disc galaxies. These elongated also believed play a crucial role secular evolutionary processes, because able efficiently redistribute gas, stars, angular momentum within their hosts, although it remains unclear as whether enhance or suppress star formation. A useful tool investigate this ambiguity is main sequence (MS) relation, which...

10.1051/0004-6361/202449894 article EN Astronomy and Astrophysics 2024-04-26
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