[:en][three_fourth last=»no» spacing=»yes» center_content=»no» hide_on_mobile=»no» background_color=» background_image=» background_image=»» background_repeat=»no-repeat» background_position=»left top» hover_type=»none» link=»» border_position=»all» border_size=»0px» border_color=» border_style=» border_style=»» padding=» margin_top=» margin_top=»» margin_bottom=» animation_type=» animation_type=»» animation_direction=»» animation_speed=»0.1″ animation_offset=» class=» class=»» id=»»][fusion_text]In 2005 I started my bachelor studies in Physics at the Universidad Católica del Norte, finishing in 2011.
Then, in 2012 I started my Master’s studies at the University of Concepción, with Dr. Matías Jones in the study of binary stars around giant stars that are candidates to host exoplanets and brown dwarfs. This study consisted in the follow-up these stars and do the characterization, finding good results which were published in A & A (2016A & A … 593A.133B).
In 2015 I started my PhD program. I working with the Professor Dr. Márcio Catelán in the calculation of accurate radial velocities for a group of stars belonging to the blue end of the horizontal branch (BHB). This type of stars belonging to the Halo, due to their nature and brightness, are excellent tracers to study the structure and kinematics of the oldest components of our Milky Way.
Research Interests
Galactic Halo BHB Stars[/fusion_text][fusion_text]
[/fusion_text][/three_fourth][one_fourth last=»yes» spacing=»yes» center_content=»no» hide_on_mobile=»no» background_color=»» background_image=»» background_repeat=»no-repeat» background_position=»left top» hover_type=»none» link=»» border_position=»all» border_size=»0px» border_color=»» border_style=»» padding=»» margin_top=»» margin_bottom=»» animation_type=»» animation_direction=»» animation_speed=»0.1″ animation_offset=»» class=»» id=»»][person name=»Paz Victoria Bluhm Ceballos» title=»» picture=»http://www.astrofisicamas.cl/wp-content/uploads/2016/11/blank.jpg» pic_link=»» linktarget=»_self» pic_style=»none» hover_type=»none» background_color=»» content_alignment=»» pic_style_color=»» pic_bordersize=»» pic_bordercolor=»» pic_borderradius=»» icon_position=»» social_icon_boxed=»» social_icon_boxed_radius=»» social_icon_color_type=»» social_icon_colors=»» social_icon_boxed_colors=»» social_icon_tooltip=»» email=»» facebook=»» twitter=»» instagram=»» dribbble=»» google=»» linkedin=»» blogger=»» tumblr=»» reddit=»» yahoo=»» deviantart=»» vimeo=»» youtube=»» pinterest=»» rss=»» digg=»» flickr=»» forrst=»» myspace=»» skype=»» paypal=»» dropbox=»» soundcloud=»» vk=»» xing=»» show_custom=»no» class=»» id=»»]E-mail: pvbluhm@uc.cl[/person][/one_fourth][:es][three_fourth last=»no» spacing=»yes» center_content=»no» hide_on_mobile=»no» background_color=» background_image=» background_image=»» background_repeat=»no-repeat» background_position=»left top» hover_type=»none» link=»» border_position=»all» border_size=»0px» border_color=» border_style=» border_style=»» padding=» margin_top=» margin_top=»» margin_bottom=» animation_type=» animation_type=»» animation_direction=»» animation_speed=»0.1″ animation_offset=» class=» class=»» id=»»][fusion_text]En el año 2005 comencé mis estudios de Licenciatura en Física en la Universidad Católica del Norte egresando el año 2011.
Luego en el año 2012 comencé mis estudios de Magíster en la Universidad de Concepción, realizando junto al Dr. Matías Jones, un estudio de estrellas binarias alrededor de estrellas gigantes que son candidatas a albergar exoplanetas y enanas cafés. El estudio consistió en el seguimiento de éstas estrellas y su posterior caracterización, encontrando buenos resultados los cuales fueron publicados en A&A (2016A&A…593A.133B).
En el año 2015 ingresé al programa de Doctorado en Astrofísica trabajando en conjunto con el profesor Dr. Márcio Catelán, en el cálculo de velocidades radiales para un grupo de estrellas pertenecientes al extremo azul de la rama horizontal (BHB). Este tipo de estrellas pertenecientes al Halo, debido a su naturaleza y brillo, son excelentes trazadores para estudiar la estructura y cinemática de los componentes mas viejos de nuestra vía láctea.
Research Interests
Galactic Halo BHB Stars[/fusion_text][fusion_text]
[/fusion_text][/three_fourth][one_fourth last=»yes» spacing=»yes» center_content=»no» hide_on_mobile=»no» background_color=»» background_image=»» background_repeat=»no-repeat» background_position=»left top» hover_type=»none» link=»» border_position=»all» border_size=»0px» border_color=»» border_style=»» padding=»» margin_top=»» margin_bottom=»» animation_type=»» animation_direction=»» animation_speed=»0.1″ animation_offset=»» class=»» id=»»][person name=»Paz Victoria Bluhm Ceballos» title=»» picture=»http://www.astrofisicamas.cl/wp-content/uploads/2016/11/blank.jpg» pic_link=»» linktarget=»_self» pic_style=»none» hover_type=»none» background_color=»» content_alignment=»» pic_style_color=»» pic_bordersize=»» pic_bordercolor=»» pic_borderradius=»» icon_position=»» social_icon_boxed=»» social_icon_boxed_radius=»» social_icon_color_type=»» social_icon_colors=»» social_icon_boxed_colors=»» social_icon_tooltip=»» email=»» facebook=»» twitter=»» instagram=»» dribbble=»» google=»» linkedin=»» blogger=»» tumblr=»» reddit=»» yahoo=»» deviantart=»» vimeo=»» youtube=»» pinterest=»» rss=»» digg=»» flickr=»» forrst=»» myspace=»» skype=»» paypal=»» dropbox=»» soundcloud=»» vk=»» xing=»» show_custom=»no» class=»» id=»»]E-mail: pvbluhm@uc.cl[/person][/one_fourth][:]
