Publication

The formation of the Milky Way halo and its dwarf satellites: A NLTE-1D abundance analysis. V. The Sextans galaxy

Related publications (37)

About
Privacy
Disclaimer

Graph Chatbot

Chat with Graph Search

Ask any question about EPFL courses, lectures, exercises, research, news, etc. or try the example questions below.

DISCLAIMER: The Graph Chatbot is not programmed to provide explicit or categorical answers to your questions. Rather, it transforms your questions into API requests that are distributed across the various IT services officially administered by EPFL. Its purpose is solely to collect and recommend relevant references to content that you can explore to help you answer your questions.

The formation of the Milky Way halo and its dwarf satellites: A NLTE-1D abundance analysis. V. The Sextans galaxy

Graph Chatbot

Chat with Graph Search

How much metal did the first stars provide to the ultra-faint dwarfs?

The extended stellar halo' of the Ursa Minor dwarf galaxy

The formation of the faintest galaxies in cosmological simulations: from the impact of primordial magnetic fields to the metal enrichment of present day dwarfs by first stars

Analysis of accretion disc structure and stability using open code for vertical structure

The Pristine survey - XV. A CHIT ESPaDOnS view on the Milky Way halo and disc populations

The first generations of stars in the Local Group

The Pristine survey - XVII. The C-19 stream is dynamically hot and more extended than previously thought

The Pristine dwarf galaxy survey - IV. Probing the outskirts of the dwarf galaxy Bootes I

Euclid: Searching for pair-instability supernovae with the Deep Survey

The formation of the milky way halo and its dwarf satellites: a NLTE-1D abundance analysis. IV. Segue 1, Triangulumii, and Coma Berenices UFDs