Fabrícia O. Barbosa

ORCID: 0000-0002-8262-2246
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About
Contact & Profiles
Research Areas
  • Stellar, planetary, and galactic studies
  • Astronomy and Astrophysical Research
  • Gamma-ray bursts and supernovae
  • Adaptive optics and wavefront sensing
  • Astronomical Observations and Instrumentation
  • Astro and Planetary Science

Museu de Astronomia e Ciências Afins
2021

Universidade de São Paulo
2021

We identified 8 additional stars as members of the Helmi stream (HStr) in combined GALAH+ DR3 and $Gaia$ EDR3 catalog. By consistently reevaluating claimed from literature, we consolidate a sample 22 HStr with parameters determined high-resolution spectroscopy spanning considerably wider (by $\sim$0.5 dex) metallicity interval ($-2.5 \lesssim \rm[Fe/H] < -1.0$) than previously reported. Our study focuses on $\alpha$ (Mg Ca) neutron-capture (Ba Eu) elements. find that chemistry is typical...

10.3847/2041-8213/ac0056 article EN The Astrophysical Journal Letters 2021-06-01

We present an updated sample of blue horizontal-branch (BHB) stars selected from the photometric and spectroscopic data Sloan Digital Sky Survey its associated project Extension for Galactic Understanding Exploration (SEGUE). With this data, we candidates A-type in color-color space then a mixture modeling technique was implemented order to distinguish between BHB main-sequence/blue-straggler based on their surface gravity values ($\log \rm{g}$) estimated by SEGUE Stellar Parameter Pipeline....

10.3847/1538-4357/ac983f article EN cc-by The Astrophysical Journal 2022-11-01

We present an updated sample of blue horizontal-branch (BHB) stars selected from the photometric and spectroscopic data Sloan Digital Sky Survey its associated project Extension for Galactic Understanding Exploration (SEGUE). With this data, we candidates A-type in color-color space then a mixture modeling technique was implemented order to distinguish between BHB main-sequence/blue-straggler based on their surface gravity values ($\log \rm{g}$) estimated by SEGUE Stellar Parameter Pipeline....

10.48550/arxiv.2210.02820 preprint EN cc-by arXiv (Cornell University) 2022-01-01
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