Seminario en Departamento de Astronomía
Susana Garay Romero 8 Jun 202108/06/21 a las 16:27 hrs.2021-06-08 16:27:08
Estimado/as
Les recuerdo que el Jueves 10 de Junio a las 10:00 hrs, tendremos seminario en el Departamento de Astronomía de la Universidad de Chile.
Speaker: Marcelo Mora
Instituto de Astrofísica, Pontificia Universidad Católica de Chile
Title: An interacting view of NGC 1427A
Abstract: NGC 1427A is a dwarf galaxy located at the outskirts of the Fornax
Galaxy Cluster. Its location, shape, and clear star
formation events have made this galaxy a nearby laboratory of how dwarfs
are affected by the dense environment of the galaxy group. The
origin of its star formation burst is unclear: It has been proposed to
be due to gravitational interaction (i.e. merger?) or ram pressure
stripping. Here I will show, in an interactive way, my latest result of
our MUSE integral field observations. I will present the advantages of
this analysis approach, drawing my final conclusion about the nature of
this galaxy. Finally, if time allows, I would like to present
further examples applied to other galaxies as work in progress.
Virtual room: uchile.zoom.us/ ... NkNpdGFZb0sxRVZJdz09
Rene A. Mendez
Seminar Coordinator
DAS/UChile - rmendez@uchile.cl
--
--
Saludos,
Alejandro Leal Obreque
Departamento de Astronomía
FCFM - UNIVERSIDAD DE CHILE
22 977 1154
aleal@das.uchile.clwww.das.uchile.cl
Les recuerdo que el Jueves 10 de Junio a las 10:00 hrs, tendremos seminario en el Departamento de Astronomía de la Universidad de Chile.
Speaker: Marcelo Mora
Instituto de Astrofísica, Pontificia Universidad Católica de Chile
Title: An interacting view of NGC 1427A
Abstract: NGC 1427A is a dwarf galaxy located at the outskirts of the Fornax
Galaxy Cluster. Its location, shape, and clear star
formation events have made this galaxy a nearby laboratory of how dwarfs
are affected by the dense environment of the galaxy group. The
origin of its star formation burst is unclear: It has been proposed to
be due to gravitational interaction (i.e. merger?) or ram pressure
stripping. Here I will show, in an interactive way, my latest result of
our MUSE integral field observations. I will present the advantages of
this analysis approach, drawing my final conclusion about the nature of
this galaxy. Finally, if time allows, I would like to present
further examples applied to other galaxies as work in progress.
Virtual room: uchile.zoom.us/ ... NkNpdGFZb0sxRVZJdz09
Rene A. Mendez
Seminar Coordinator
DAS/UChile - rmendez@uchile.cl
--
--
Saludos,
Alejandro Leal Obreque
Departamento de Astronomía
FCFM - UNIVERSIDAD DE CHILE
22 977 1154
aleal@das.uchile.clwww.das.uchile.cl
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| Última Modificación | 8 Jun 202108/06/21 a las 16:27 hrs.2021-06-08 16:27:08 |
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