Dr. GERARDO RAMOS LARIOS
Resumen curricular:
Investigador Titular C en el Instituto de Astronomía y Meteorología del Física. Es Investigador Nivel 2 del Sistema Nacional de Investigadores, miembro de la Academia Mexicana de Ciencias, de la Unión Astronómica Internacional y de la American Astronomical Society. Ha publicado más de 100 artículos JCR y recibido varios reconocimientos, entre los cuales destacan la Presea al Mérito Académico en 2021, la Cátedra de Investigación Marcos Moshinsky en 2017, el Premio Estatal de Ciencia Tecnología e Innovación de Jalisco en 2 ocasiones (2013 y 2010) y fue ganador en los concursos nacionales de Fotografía Científica en 2008, 2009, 2010 y 2020 de CONACyT. Su campo de estudio es la Astrofísica del Medio Interestelar, con especialidad en Astronomía Infrarroja.
Perfil de Investigador SNII:
Perfil PRODEP:
Bases de datos bibliográficas:
Scopus
ORCID
Publicaciones del académico:
- Shaping the nebula around the symbiotic system R Aquarii
- 3D physical structure and angular expansion of the remnant of the recurrent nova TPyx
- Chemical abundances and ionizing mechanisms in the star-forming double-ring of AM 0644-741 using MUSE data
- H2 molecular gas in the old planetary nebula NGC 3587
- NGC 2022, a case study of a multiple-shell planetary nebula
- Emerging planetary nebulae within 3D spiral patterns
- Planetary nebulae with Wolf-Rayet-type central stars - IV. NGC 1501 and its mixing layer
- QU Vul: An integral field spectroscopy case study of a nova shell
- Adjusting the bow-tie: a morpho-kinematic study of NGC 40
- Common envelope evolution in born-again planetary nebulae - Shaping the H-deficient ejecta of A 30
- Nebular abundance gradient in the Cartwheel galaxy using MUSE data
- The Common Envelope Origins of the Fast Jet in the Planetary Nebula M 3-38
- 3D mapping of the Wolf-Rayet nebula M 1-67: Clues for post-common envelope evolution in massive stars
- Rings and arcs around evolved stars - III. Physical conditions of the ring-like structures in the planetary nebula IC 4406 revealed by MUSE
- Exploitation of the IPHAS to Investigate Planetary Nebulae
- Spatiokinematic models of five nova remnants: Correlations between nova shell axial ratio, expansion velocity, and speed class
- Millimetre Observations of Maser-Emitting Planetary Nebulae
- An XMM-Newton EPIC X-Ray View of the Symbiotic Star R Aquarii
- Erratum: Planetary nebulae with Wolf-Rayet-type central stars-II. Dissecting the compact planetary nebula M 2-31 with GTC MEGARA (Monthly Notices of the Royal Astronomical Society (2021) 508 (2254-2265) DOI: 10.1093/mnras/stab2531)
- Planetary nebulae with Wolf-Rayet-type central stars - III. A detailed view of NGC 6905 and its central star
- Planetary nebulae with Wolf-Rayet-type central stars - II. Dissecting the compact planetary nebula M 2-31 with GTC MEGARA
- First deep images catalogue of extended IPHAS PNe
- Carbon dust in the evolved born-again planetary nebulae A 30 and A 78
- X-ray observations of the nova shell IPHASX J210204.7+471015
- Tomography of the Unique Ongoing Jet in the Planetary Nebula NGC 2392
- Detailed studies of IPHAS sources - I. The disrupted late bipolar IPHASX J193718.6+202102
- Detailed studies of IPHAS sources - II. Sab 19, a true planetary nebula and its mimic crossing the Perseus Arm
- Detailed studies of IPHAS sources - III. The highly extinguished bipolar planetary nebula IPHASX J191104.8+060845
- On the Contribution of the X-Ray Source to the Extended Nebular HeII Emission in IZW18
- The Decline and Fall of the Youngest Planetary Nebula
- Unveiling the stellar origin of the Wolf-rayet nebula NGC6888 through infrared observations
- Discovery of a Fast-expanding Shell in the Inside-out Born-again Planetary Nebula HuBi 1 through High-dispersion Integral Field Spectroscopy
- Planetary nebulae with Wolf-Rayet-type central stars-I. the case of the high-excitation NGC 2371
- Rings and arcs around evolved stars – II. The carbon star AFGL 3068 and the planetary nebulae NGC 6543, NGC 7009, and NGC 7027
- Rings and arcs around evolved stars – II. The carbon star AFGL 3068 and the planetary nebulae NGC 6543, NGC 7009, and NGC 7027
- Molecular hydrogen microstructures in planetary nebulae
- The Bubble Nebula NGC 7635-Testing the wind-blown bubble theory
- H2 emission in the low-ionization structures of the planetary nebulae NGC 7009 and NGC 6543
- Angular Expansion of Nova Shells
- Dark matter content of ETGs and its relation to the local density of galaxies
- Extended X-ray emission from the classic nova DQ Her – on the possible presence of a magnetized jet
- Extended X-ray emission from the classic nova DQ Her – on the possible presence of a magnetized jet
- Application of Artificial Neural Networks for the Automatic Spectral Classification
- The quantity of dark matter in early-type galaxies and its relation to the environment
- A machine learning approach for identification and classification of symbiotic stars using 2MASS and WISE
- Measuring the expansion and age of the nova shell IPHASX J210204.7 + 471015
- Hidden IR structures in NGC 40: Signpost of an ancient born-again event
- A Census of Symbiotic Stars in the 2MASS, WISE, and Gaia Surveys
- Pilot program with the LMT to look for molecules in Planetary nebulae
- Rapidly evolving episodic outflow in IRAS 18113-2503: Clues to the ejection mechanism of the fastest water fountain