$R_{\rm e}$. II. Understanding the IC 3475 galaxy type, including ultra-diffuse galaxy, structural scaling relations

Ähnliche Einträge

• Repainting the colour-mass diagrams by unearthing the green mountain: dust-rich S0 galaxies in the colour-(galaxy stellar mass) diagram, and the colour-(black hole mass) relations for dust-poor versus dust-rich galaxies
  von: Graham, Alister W.
  Veröffentlicht: (2024)
• Elliptical (E) and ellicular (ES) galaxies in the M_bh-M_*,sph diagram, and a merger-driven explanation for the origin of ES galaxies, anti-truncated stellar discs in lenticular galaxies, and the Sersicification of E galaxy light profiles
  von: Graham, Alister W.
  Veröffentlicht: (2025)
• Dot to dot: high-$z$ little red dots in $M_{\rm bh}$-$M_{\rm \star}$ diagrams with galaxy-morphology-specific scaling relations
  von: Graham, Alister W., et al.
  Veröffentlicht: (2025)
• Clash of the Trident and Tuning Fork: insights from bar and spiral strength in the (massive black hole)-stellar mass diagrams, and the `Triangal' galaxy evolution schema
  von: Graham, Alister W.
  Veröffentlicht: (2026)
• Simulations of cluster ultra-diffuse galaxies in MOND
  von: Nagesh, Srikanth T., et al.
  Veröffentlicht: (2024)