
Dr. RAMIRO FRANCO HERNÁNDEZ
Resumen curricular:
El Dr. Ramiro Franco Hernández recibió su Doctorado en Ciencias (Astronomía) en la Universidad Nacional Autónoma de México y realizó posdoctorados en Astrofísica en el Max Planck Institute fuer Radioastronomie de Alemania y Departamento de Astronomía de la Universidad de Chile. Actualmente es Profesor e Investigador del Instituto de Astronomía y Meteorología adscrito al Centro UniversitEs miembro del Sistema Nacional de Investigadores (SNI), con Nivel I desde el año 2014. A lo largo de su carrera científica, ha publicado 25 artículos indexados en el Journal Citation Reports (JCR). Como investigador, ha participado en más de 10 congresos nacionales e internacionales. Dentro de sus actividades, destaca la divulgación de la ciencia en todos sus niveles, con más de 40 charlas y talleres.ario de Ciencias Exactas e Ingenierías, de la Universidad de Guadalajara. Su campo de estudio dentro de la Física es la Astrofísica, en especial la formación estelar utilizando observaciones en ondas de radio (radioastronomía) y simulaciones numéricas.
Enlaces
Perfil de Investigador SNII:
Perfil PRODEP:
Bases de datos bibliográficas:
Publicaciones del académico:
- Can envelope backwarming of discs explain mm-bright, extended protostellar structures?
- A Census of the Low Accretors. II. Accretion Properties
- Dusty mm-bright protostellar structures
- JWST Detects Neon Line Variability in a Protoplanetary Disk
- A multiwavelength study of protoplanetary disk ionization
- Searching for Evidence of EUV Photoevaporation in Actively Dispersing Protoplanetary Disks
- Testing the Potential for Radio Variability in Disks around T Tauri Stars with Observations and Chemical Modeling
- VizieR Online Data Catalog: T Tauri star IR excesses & Ha eq. widths (Manzo-Martinez+, 2020)
- Accretion in the PDS 70 system
- The Evolution of the Inner Regions of Protoplanetary Disks
- Variable Accretion onto Protoplanet Host Star PDS 70
- Magnetospheric Accretion as a Source of Hα Emission from Protoplanets around PDS 70
- Complex Magnetospheric Accretion Flows in the Low Accretor CVSO 1335
- Magnetospheric accretion as a source of Hα emission from protoplanets around PDS 70
- An Incipient Debris Disk in the Chamaeleon I Cloud
- The tidal filament of NGC 4660
- ALMA reveals a candidate hot and compact disc around the O-type protostar IRAS 16547-4247
- THE 2014 ALMA LONG BASELINE CAMPAIGN: AN OVERVIEW
- An Overview of the 2014 ALMA Long Baseline Campaign
- ALMA reveals a candidate hot and compact disc around the O-type protostar IRAS 16547− 4247
- The magnetic field toward the young planetary nebula K 3-35
- The rotating molecular structures and the ionized outflow associated with IRAS 16547-4247
- Hypercompact h ii regions: Resolved images of g34.26+0.15 a and b
- The collimated jet source in Iras 16547-4247: Time variation, possible precession, and upper limits to the proper motions along the jet axis
- HCO+ emission possibly related with a shielding mechanism that protects water molecules in the young PN K 3-35
- Detection of HCO+ emission toward the planetary nebula K3-35
- Discovery of an energetic bipolar molecular outflow towards IRAS 16547-4247
- A survey and analysis of Spitzer infrared spectrograph spectra of T Tauri stars in Taurus
- Spectra and sizes of hypercompact H II regions
- Effects of dust growth and settling in T tauri disks
- Disks in transition in the Taurus population: Spitzer irs spectra of GM aurigae and DM tauri
- IRAC observations of taurus pre-main-sequence stars
- The truncated disk of CoKu Tau/4