Scientific Results
- Positions for CIG galaxies
- Redshift and distances
- Morphologies
- Optical refinement
- Photometric characterization of Sb-Sc galaxies
- Fourier Photometric Analysis of ∼100 AMIGA galaxies
- Comprehensive Examination of the..
- Isolation
- A catalogue of neighbours around isolated galaxies based on POSS I & II images
- Quantification of isolation based on POSS I & II images
- Revision of isolation criteria using the SDSS
- Effects of the environment on galaxies in the..
- Catalogues of isolated galaxies, isolated pairs, and isolated triplets..
- Star formation
- Isolated Galaxies
- Infrared Diagnostics
- Hα study of a redshift-limited subsample
- Star formation in bars
- Star formation in outer disks
- Optical colours of isolated galaxies
- Compact Groups
- Isolated Galaxies
- Optical specialization
- First optical specialization of the CIG
- The stellar mass-size relation for isolated galaxies
- Are (pseudo) bulges in isolated galaxies actually primordial relics?
- Linking the sub-kpc scales with the environment of galaxies..
- Radio continuum properties
- Atomic gas
- Isolated Galaxies
- Environment and faint features of CIG 96: deep optical and HI observations (2018)
- Atomic gas scaling relations (2018)
- A ∼12 kpc HI extension and other HI asymmetries in the isolated galaxy CIG 340 (2014)
- HI asymmetry in the isolated galaxy CIG 85 (2012)
- HI asymmetries in the isolated galaxy CIG 292 (2011)
- Asymmetries in isolated galaxies (2011)
- The large asymmetric HI envelope of CIG 96 (2005)
- Compact groups
- Evolution in compact groups: The HI content of Hickson Compact Group 16 (2019)
- Distribution of faint atomic gas in Hickson Compact Groups using GBT data (2015)
- Studies of complementary samples
- Isolated Galaxies
- Molecular gas
- Isolated Galaxies
- Compact Groups
- Strong far-infrared cooling lines, peculiar CO kinematics, and possible star-formation suppression in Hickson Compact Group 57
- Star formation suppression in compact group galaxies: a new path to quenching?
- Nuclear activity
- Far-infrared and radio continuum study of nuclear activity
- Optical characterization of the nuclear activity
Isolated galaxies
CO molecular gas content
CO molecular gas content We have CO(1-0) data for 273 AMIGA galaxies, most of them (n=186) from our own observations with the IRAM 30m and...
Chemistry in isolation
Chemistry in isolation Molecular abundances in the ISM have been shown to be imprinted by the different activity types in the nuclear region of galaxies....
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Compact groups
Strong far-infrared cooling lines, peculiar CO kinematics, and possible star-formation suppression in Hickson Compact Group 57
Strong far-infrared cooling lines, peculiar CO kinematics, and possible star-formation suppression in Hickson Compact Group 57 In this work, [C II] and [O I] observations...
Star formation suppression in compact group galaxies: a new path to quenching?
Star formation suppression in compact group galaxies: a new path to quenching? In the current work CO(1–0) maps of 12 warm H2-selected Hickson Compact Groups...
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