Analysis of the interstellar Medium of Isolated GAlaxies
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Instituto de Astrofísica de Andalucía
CSIC
AMIGA
About AMIGA
What we do
Who we are
Scientific Results
Positions
Redshift and distances
Morphologies
Isolation
Star formation
Optical specialization
Radio continuum properties
Atomic gas
Molecular gas
Nuclear activity
Technological Developments
Distributed Computing
Participation in the SKA
Reproducible science
The Virtual Observatory archives and tools
Funded Projects
Ongoing projects
Previous projects
Publications
Refereed papers
PhD Theses
Master Theses
Organised events
ASCII files
Menu
About AMIGA
What we do
Who we are
Scientific Results
Positions
Redshift and distances
Morphologies
Isolation
Star formation
Optical specialization
Radio continuum properties
Atomic gas
Molecular gas
Nuclear activity
Technological Developments
Distributed Computing
Participation in the SKA
Reproducible science
The Virtual Observatory archives and tools
Funded Projects
Ongoing projects
Previous projects
Publications
Refereed papers
PhD Theses
Master Theses
Organised events
ASCII files
Home
Publications
On the nature of faint mid-infrared sources in M 33
Publications
Refereed papers
Statistical studies of the AMIGA sample
Individual studies of isolated galaxies
Studies of complementary samples
Star formation, interstellar medium and nuclear activity in complementary environments
Physico-chemical conditions of the molecular gas
Blind HI samples
Publications on technological developments
PhD theses
Master’s theses
Refereed papers
Statistical studies of the AMIGA sample
Individual studies of isolated galaxies
Studies of complementary samples
Star formation, interstellar medium and nuclear activity in complementary environments
Physico-chemical conditions of the molecular gas
Blind HI samples
Publications on technological developments
PhD theses
Master’s theses
December 26, 2011
E. Corbelli, C. Giovanardi, F. Palla, and S. Verley.
2011 A&A 528, 116
Instituto de Astrofísica de Andalucía
E. Corbelli, C. Giovanardi, F. Palla, and S. Verley.E. Corbelli, C. Giovanardi, F. Palla, and S. Verley.