Publication

IFUM integrated field spectroscopy of ten M104 satellite galaxy candidates

Oliver Müller
2024

Abstract

We report the spectroscopic analysis of 10 satellite galaxy candidates in the sphere of influence of the Sombrero galaxy (M104, NGC4594), based on data obtained with IFUM (integral field units for Magellan). Based on their newly observed recessional velocities, we confirm that nine of these candidates are satellite galaxies of M104, with one being a background dwarf galaxy. All 10 dwarfs have stellar masses 2x10(7) to 1x10(9)M(circle dot) and mean weighted metallicities -1.7

Official source

https://infoscience.epfl.ch/entities/publication/482657db-aa13-4803-8054-7d2a6e1be5ff

About this result

This page is automatically generated and may contain information that is not correct, complete, up-to-date, or relevant to your search query. The same applies to every other page on this website. Please make sure to verify the information with EPFL's official sources.

Graph Chat

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.

IFUM integrated field spectroscopy of ten M104 satellite galaxy candidates

Chat with Graph Search

The AGORA High-Resolution Galaxy Simulations Comparison Project VII. Satellite quenching in zoom-in simulation of a Milky Way-mass halo

Euclid: Early Release Observations – Deep anatomy of nearby galaxies

Euclid: Early Release Observations of diffuse stellar structures and globular clusters as probes of the mass assembly of galaxies in the Dorado group?