C. Román-Zúñiga

Ensenada Institute of Technology — Mexico

Physics and Astronomy · Physical Sciences

31h-index7.2kcitations291works2.42yr avg
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Research Topics

Gamma-ray bursts and supernovae(151), SAS software applications and methods(111), Stellar, planetary, and galactic studies(104), Astrophysics and Star Formation Studies(88), Astronomy and Astrophysical Research(57)

Publications284 total

SDSS-V LVM: Resolving physical conditions in the Trifid Nebula
Astronomy and Astrophysics·2025· 1 citedOpen Access
SDSS-V LVM: Resolving Physical Conditions in the Trifid Nebula
arXiv (Cornell University)·2025Open Access
The large-scale kinematics of young stars in the Milky Way disc: First results from SDSS-V
Astronomy and Astrophysics·2025Open Access
SDSS-V Local Volume Mapper (LVM): revealing the structure of the Rosette Nebula
Monthly Notices of the Royal Astronomical Society·2025· 1 citedOpen Access
The large-scale kinematics of young stars in the Milky Way disc: first results from SDSS-V
ArXiv.org·2025Open Access
Atmospheric parameters and chemical abundances of young stars with APOGEE – I. Orion star-forming region
Monthly Notices of the Royal Astronomical Society·2025Open Access
How Massive Star Clusters Form and Evolve: A Near-IR Survey of the W51 Complex
The Astronomical Journal·2025Open Access
How Massive Star Clusters Form and Evolve: A Near-IR Survey of the W51 Complex
arXiv (Cornell University)·2025Open Access
ABYSS. III. Observing Accretion Activity in Young Stars Through Empirical Veiling Measurements
The Astronomical Journal·2025· 1 citedOpen Access
Gravity or turbulence? – VII. The Schmidt–Kennicutt law, the star formation efficiency, and the mass density of clusters from gravitational collapse rather than turbulent support
Monthly Notices of the Royal Astronomical Society·2025Open Access
ABYSS III: Observing accretion activity in young stars through empirical veiling measurements
arXiv (Cornell University)·2025Open Access
Testing the bloated star hypothesis in the massive young stellar object IRAS 19520+2759 through optical and infrared variability
Monthly Notices of the Royal Astronomical Society·2025Open Access
Testing the bloated star hypothesis in the massive young stellar object IRAS 19520+2759 through optical and infrared variability
arXiv (Cornell University)·2025Open Access
Kinematic study of the Orion Complex: analysing the young stellar clusters from big and small structures
Monthly Notices of the Royal Astronomical Society·2024· 6 citedOpen Access
Gravity or turbulence? VII. The Schmidt-Kennicutt law, the star formation efficiency, and the mass density of clusters from gravitational collapse rather than turbulent support
arXiv (Cornell University)·2024· 2 citedOpen Access
Kinematic study of the Orion Complex: Analysing the young stellar clusters from big and small structures
arXiv (Cornell University)·2024Open Access
Gravity or turbulence? VI. The physics behind the Kennicutt-Schmidt relations
arXiv (Cornell University)·2024Open Access
Gravity or turbulence? – VI. The physics behind the Kennicutt–Schmidt relation
Monthly Notices of the Royal Astronomical Society·2024· 4 citedOpen Access
SDSS-V Local Volume Mapper (LVM): A glimpse into Orion
Astronomy and Astrophysics·2024· 20 citedOpen Access
Atmospheric parameters and chemical abundances within 100 pc: a sample of G, K, and M main-sequence stars
Monthly Notices of the Royal Astronomical Society·2024· 5 citedOpen Access
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Frequent Co-authors

Jesús Hernández(12), A. M. Watson(12), A. Kutyrev(12), Kevin R. Covey(11), M. G. Richer(11), Marina Kounkel(10), J. S. Bloom(10), J. González‐Hernández(10), J. X. Prochaska(10), Alexandre Roman–Lopes(9), N. Butler(9), Elizabeth A. Lada(9), J. Alves(9), Keivan G. Stassun(8), Guy S. Stringfellow(8), William H. Lee(8), C. J. Lada(8), J. A. de Diego(8), O. Fox(8), E. Ramírez-Ruiz(7)