Environment and self-regulation in galaxy formation
The environment is known to affect the formation and evolution of galaxies considerably best
visible through the well-known morphology–density relationship. It is less clear, though …
visible through the well-known morphology–density relationship. It is less clear, though …
[PDF][PDF] Environment and self-regulation in galaxy formation
D Thomas, C Maraston, K Schawinski… - arXiv preprint arXiv …, 2009 - core.ac.uk
The environment is known to affect the formation and evolution of galaxies considerably best
visible through the well-known morphology-density relationship. It is less clear, though …
visible through the well-known morphology-density relationship. It is less clear, though …
Environment and self-regulation in galaxy formation
D Thomas, C Maraston, K Schawinski… - Monthly Notices of …, 2010 - ieeexplore.ieee.org
The environment is known to affect the formation and evolution of galaxies considerably best
visible through the well-known morphology–density relationship. It is less clear, though …
visible through the well-known morphology–density relationship. It is less clear, though …
Environment and self‐regulation in galaxy formation
D Thomas, C Maraston, K Schawinski… - Monthly Notices of …, 2010 - Wiley Online Library
The environment is known to affect the formation and evolution of galaxies considerably best
visible through the well‐known morphology–density relationship. It is less clear, though …
visible through the well‐known morphology–density relationship. It is less clear, though …
Environment and self-regulation in galaxy formation
D Thomas, C Maraston, K Schawinski… - Monthly Notices of the …, 2010 - uhra.herts.ac.uk
The environment is known to affect the formation and evolution of galaxies considerably best
visible through the well-known morphology–density relationship. It is less clear, though …
visible through the well-known morphology–density relationship. It is less clear, though …
[PDF][PDF] Environment and self-regulation in galaxy formation
D Thomas, C Maraston, K Schawinski, M Sarzi… - Mon. Not. R. Astron …, 2010 - icg.port.ac.uk
The environment is known to affect the formation and evolution of galaxies considerably best
visible through the well-known morphology–density relationship. It is less clear, though …
visible through the well-known morphology–density relationship. It is less clear, though …
Environment and self-regulation in galaxy formation
D Thomas, C Maraston, K Schawinski, M Sarzi… - arXiv preprint arXiv …, 2009 - arxiv.org
The environment is known to affect the formation and evolution of galaxies considerably best
visible through the well-known morphology-density relationship. In this paper we study the …
visible through the well-known morphology-density relationship. In this paper we study the …
[PDF][PDF] Environment and self-regulation in galaxy formation
D Thomas, C Maraston, K Schawinski, M Sarzi… - arXiv preprint arXiv …, 2009 - Citeseer
The environment is known to affect the formation and evolution of galaxies considerably best
visible through the well-known morphology-density relationship. It is less clear, though …
visible through the well-known morphology-density relationship. It is less clear, though …
Environment and self‐regulation in galaxy formation
D Thomas, C Maraston, K Schawinski, M Sarzi… - Monthly Notices of the …, 2010 - infona.pl
The environment is known to affect the formation and evolution of galaxies considerably best
visible through the well‐known morphology–density relationship. It is less clear, though …
visible through the well‐known morphology–density relationship. It is less clear, though …
[引用][C] Environment and self-regulation in galaxy formation
D THOMAS, C MARASTON… - Monthly notices of …, 2010 - pascal-francis.inist.fr
Environment and self-regulation in galaxy formation CNRS Inist Pascal-Francis CNRS
Pascal and Francis Bibliographic Databases Simple search Advanced search Search by …
Pascal and Francis Bibliographic Databases Simple search Advanced search Search by …