The Tully-Fisher relation in dense groups at $z \sim 0.7$ in the MAGIC survey

Galaxies in dense environments are subject to interactions and mechanisms which directly affect their evolution by lowering their gas fractions and reducing their star-forming capacity earlier than their isolated counterparts. The aim of our project is to get new insights about the role of environment on the stellar and baryonic content of galaxies using a kinematic approach, through the study of the Tully-Fisher relation (TFR). We study a sample of galaxies in 8 groups spanning a redshift range of $0.5

Keywords:

• Physics
• Astrophysics
• Galaxy
• Tully–Fisher relation
• Stellar mass
• Star formation
• Baryon
• Emission spectrum
• Redshift
• Mass distribution

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