Man

Samer - Kanaan -

staff

universidad de valparaiso

valparaiso, Chile

Líneas de Investigación


Hot active stars, Be stars, B[e] stars, Yellow hyoergiants,stellar interferometry, spectroscopy, multi-technique observations, radiative transfer.

Educación

  •  Astrophysics, UNIVERSITE DE NICE-SOPHIA ANTIPOLIS. Francia, 2010
  •  Astrophysics, UNIVERSITE DE NICE-SOPHIA ANTIPOLIS. Francia, 2006

Experiencia Académica

  •   staff Full Time

    UNIVERSIDAD DE VALPARAISO

    ciencia

    valparaiso, Chile

    2013 - At present

Experiencia Profesional

  •   staff Full Time

    universidad de valparaiso

    valparaiso, Chile

    2013 - At present

Formación de Capital Humano


1- Tesis:

- Ph.D. of Catalina Arcos Carvajal (2014)
Title : to be defined
- Master tesis of Catalina Arcos Carvajal (2012)
title : modeling of Be and B[e] stars.
- Pregraduate thesis of Catalina Arcos Carvajal (2011)
title : SIMECA: Modeling the gas envelope of the B[e] HD 45677
- Pregraduate thesis of Catalina Arcos Carvajal(2010)
title : Implementacion del codigo MC3D: Aplicacion a la estrella B[e] HD 45677.

2- Teaching :

• Stellar interferometry (Master)
• IDL (Licence)
• Astrostatistics (Licence)
• Stellar atmosphere (Master)

3- Organizer of the First VLTI School in Chile Valparaiso (3-7 November 2014)

4- Member of the CNTAC comite.



 

Article (10)

The yellow hypergiant HR 5171 A: Resolving a massive interacting binary in the common envelope phase
First spectro-interferometric survey of Be stars I. Observations and constraints on the disk geometry and kinematics
Observational constraints for the circumstellar disk of the B[e] star CPD-52 9243
Imaging the spinning gas and dust in the disc around the supergiant A[e] star HD 62623
The binary Be star delta Scorpii at high spectral and spatial resolution I. Disk geometry and kinematics before the 2011 periastron
Resolving the dusty circumstellar environment of the A[e] supergiant HD 62623 with the VLTI/MIDI
The environment of the fast rotating star Achernar
Disk and wind evolution of Achernar: the breaking of the fellowship
SIMECA: a Code Dedicated to Active Hot Stars
Be stars: one ring to rule them all?

ConferenceProceedingWhole (6)

CPD-52 9243: Circumstellar Dust and Gas Properties Derived from Interferometric and Spectroscopic Data
Observational Constraints on the Disk Size and Kinematics of HD 327083*
Stars with the B[e] phenomenon seen by long baseline interferometry
δ Sco 2011 Periastron Passage: Near-IR Interferometry and Radio mm Observations
The complex environment of the fast rotating star Achernar
Disk and wind evolution of the fast rotator Achernar.
18
Samer Kanaan

staff

fisica y astronomia

universidad de valparaiso

valparaiso, Chile

2
Michel Cure

FULL PROFESSOR

Facultad de Ciencias

UNIVERSIDAD DE VALPARAISO, FACULTAD DE CIENCIAS, INSTITUTO DE FISICA Y ASTRONOMIA

Valparaiso, Chile

1
Leonardo Vanzi

full time

Electrical Engineering

Pontificia Universidad Catolica de Chile

Santiago, Chile

1
Catalina Arcos

Professor

Instituto de Física y Astronomía

Valparaíso, Chile