Man

Manuel Antonio Merello Ferrada

Investigador Adjunto

Pontificia Universidad Católica de Chile

Santiago, Chile

Líneas de Investigación


Educación

  •  Astronomy, UNIVERSITY OF TEXAS AT AUSTIN. Estados Unidos, 2014
  •  Astronomía, UNIVERSIDAD DE CHILE. Chile, 2008
  •  Astronomía, UNIVERSIDAD DE CHILE. Chile, 2005
  •  Física, UNIVERSIDAD DE CHILE. Chile, 2005

Experiencia Profesional

  •   Astrónomo soporte para telescopio APEX Other

    Agencia Nacional de Investigación y Desarrollo

    Santiago, Chile

    2019 - 2025

  •   Investigador postdoctoral Other

    Universidad de Chile

    Santiago, Chile

    2019 - 2025

  •   Investigador postdoctoral Full Time

    Universidade de Sao Paulo

    Sao Paulo, Brasil

    2018 - 2019

  •   Investigador postdoctoral Full Time

    Istituto di Astrofisica e Planetologia Spaziali - INAF

    Roma, Italia

    2014 - 2017


 

Article (23)

ALMAGAL I. The ALMA evolutionary study of high-mass protocluster formation in the Galaxy: Presentation of the survey and early results
ALMAGAL II. The ALMA evolutionary study of high-mass protocluster formation in the Galaxy: ALMA data processing and pipeline
ATOMS: ALMA three-millimetre observations of massive star-forming regions-XVII. High-mass star-formation through a large-scale collapse in IRAS 15394-5358
Dynamical accretion flows ALMAGAL: Flows along filamentary structures in high-mass star-forming clusters
Revisiting the massive star-forming complex RCW 122: New millimeter and submillimeter study
Observations and Chemical Modeling of the Isotopologues of Formaldehyde and the Cations of Formyl and Protonated Formaldehyde in the Hot Molecular Core G331.512-0.103
A Spectral Survey of CH3CCH in the Hot Molecular Core G331.512-0.103
The Star Formation Rate of the Milky Way as Seen by Herschel
Distance of Hi-GAL sources
Isocyanic acid (HNCO) in the hot molecular core G331.512-0.103: Observations and chemical modelling
The Hi-GAL compact source catalogue - II. The 360° catalogue of clump physical properties
Which Molecular Cloud Structures Are Bound?
The Hi-GAL catalogue of dusty filamentary structures in the Galactic plane
ALMA Observations of the Massive Molecular Outflow G331.512-0.103. II. Physical Properties, Kinematics, and Geometry Modeling
Cyanoacetylene in the outflow/hot molecular core G331.512-0.103
Thermal balance and comparison of gas and dust properties of dense clumps in the Hi-GAL survey
G331.512-0.103: An Interstellar Laboratory for Molecular Synthesis. I. The Ortho-to-para Ratios for CH3OH and CH3CN
THE BOLOCAM GALACTIC PLANE SURVEY. XI. TEMPERATURES AND SUBSTRUCTURE OF GALACTIC CLUMPS BASED ON 350 μM OBSERVATIONS
ALMA OBSERVATIONS OF THE MASSIVE MOLECULAR OUTFLOW G331.512-0.103
AN ANALYSIS OF THE ENVIRONMENTS OF FU ORIONIS OBJECTS WITH HERSCHEL
PHYSICAL CHARACTERISTICS OF G331.5-0.1: THE LUMINOUS CENTRAL REGION OF A GIANT MOLECULAR CLOUD
DISENTANGLING THE ENVIRONMENT OF THE FU ORIONIS CANDIDATE HBC 722 WITH HERSCHEL
Discovery of an extremely high velocity, massive, and compact molecular outflow in Norma

ConferencePaper (1)

ALMA Observations of the Massive Molecular Outflow G331.512-0.103: Physical Properties, Kinematics and Geometry Modelling

Review (1)

Molecular cloud catalogue from 13CO (1-0) data of the Forgotten Quadrant Survey
13
Leonardo Bronfman

Full Professor

Astronomy

UNIVERSIDAD DE CHILE, FACULTAD DE CIENCIAS FÍSICAS Y MATEMÁTICAS

Santiago, Chile

2
Diego Mardones

profesor asociado

astronomia

UNIVERSIDAD DE CHILE

Santiago, Chile

3
Ricardo Finger

Associate Professor

Astronomy

Universidad de Chile

Santiago, Chile

5
Guido Garay

Profesor Titular

Astronomy

Universidad de Chile

Santiago, Chile

1
Amelia Stutz

Associate Professor

Astronomy

UNIVERSIDAD DE CONCEPCION

Concepcion, Chile

1
Carlos Hervías

FONDECYT postdoctoral fellow

Instituto de Astrofisica

Pontificia Universidad Católica de Chile

Santiago, Chile

25
Manuel Merello

Investigador Adjunto

Centro de Astro-Ingeniería

Pontificia Universidad Católica de Chile

Santiago, Chile