. The bottom panel shows the mean spatial distribution of these two inner Galaxy stellar traces. The red-clump stars studied in Gonzalez et al. (2012) [98] to trace the bar/bulge are shown as triangles. " caption_title_tag="2" fusion_font_family_caption_title_font="" fusion_font_variant_caption_title_font="" caption_title_size="" caption_title_line_height="" caption_title_letter_spacing="" caption_title_transform="" caption_title_color="" caption_background_color="" fusion_font_family_caption_text_font="" fusion_font_variant_caption_text_font="" caption_text_size="" caption_text_line_height="" caption_text_letter_spacing="" caption_text_transform="" caption_text_color="" caption_border_color="" caption_overlay_color="" caption_margin_top="" caption_margin_right="" caption_margin_bottom="" caption_margin_left="" animation_type="" animation_direction="left" animation_color="" animation_speed="0.3" animation_delay="0" animation_offset="" filter_hue="0" filter_saturation="100" filter_brightness="100" filter_contrast="100" filter_invert="0" filter_sepia="0" filter_opacity="100" filter_blur="0" filter_hue_hover="0" filter_saturation_hover="100" filter_brightness_hover="100" filter_contrast_hover="100" filter_invert_hover="0" filter_sepia_hover="0" filter_opacity_hover="100" filter_blur_hover="0"]https://www.oato.inaf.it/wp-content/uploads/2025/02/250211.On-the-use-of-field-RR-Lyrae-to-constrain-the-early-formation-of-the-Galactic-spheroid.png "field RR Lyrae")
field RR Lyrae
Giuseppe Bono
Giovedì 19 Febbraio 2025, H 11.00 AM
Aula Verde Dept. Physics – Via Pietro Giuria, 1 10125 Torino
LIVE STREAMING
Abstract
RR Lyrae are low-mass radial variables and they can be used as tracers of old (t>10 Gy) stellar populations and accurate primary distance indicators.
During the last few years they have been the cross-road of several photometric and spectroscopic investigations and they have been identified not only in the Galactic components hosting old stellar populations (Halo, Bulge), but also on the Thin disk.
This circumstantial evidence opens the path to new views concerning the early formation of the Galactic spheroid.
We discuss recent findings based on kinematic data (proper motion, distance) provided by Gaia and on ground-based spectroscopic data (radial velocities, abundances) of field RR Lyrae.
Moreover, we plan to discuss the identification of stellar streams and the impact that major/minor accretion events have had on the mass assembly of the Milky Way.
Referente locale: Antonaldo Diaferio
