I review the insights emerging from recent large kinematic surveys of galaxies at low redshift, with particular reference to the SAMI, CALIFA and MaNGA surveys. These new observations provide a more comprehensive picture of the angular momentum properties of galaxies over wide ranges in mass, morphology and environment in the present-day universe. I focus on the distribution of angular momentum within galaxies of various types and the relationship between mass, morphology and specific angular momentum. I discuss the implications of the new results for models of galaxy assembly
We investigate the stellar angular momentum of galaxies across the Hubble sequence from the CALIFA s...
We study 379 central and 159 satellite early-type galaxies with two-dimensional kinematics from the ...
The “kinematic” morphology–density relation for early-type galaxies posits that those galaxies with ...
I review the insights emerging from recent large kinematic surveys of galaxies at low redshift, with...
Studying the build-up of mass and angular momentum in galaxies is fundamental to understanding the l...
We investigate the relationship between stellar and gas specific angular momentum j, stellar mass M⁎...
We investigate the relationship between stellar and gas specific angular momentum j, stellar massM* ...
Aims. At intermediate redshift, galaxy groups and clusters are thought to impact galaxy properties s...
Aims. At intermediate redshift, galaxy groups and clusters are thought to impact galaxy properties s...
We study the spatially resolved stellar specific angular momentum j* in a high-quality sample of 24 ...
We measure λRe, a proxy for galaxy specific stellar angular momentum within one effective radius, an...
We measure λRe, a proxy for galaxy specific stellar angular momentum within one effective radius, an...
Context. Galaxy formation in the current cosmological paradigm is a very complex process in which in...
Angular momentum (AM) is a key parameter to understand galaxy formation and evolution. AM originates...
Galaxy formation is a very complex process in which many different physical mechanisms intervene. Wi...
We investigate the stellar angular momentum of galaxies across the Hubble sequence from the CALIFA s...
We study 379 central and 159 satellite early-type galaxies with two-dimensional kinematics from the ...
The “kinematic” morphology–density relation for early-type galaxies posits that those galaxies with ...
I review the insights emerging from recent large kinematic surveys of galaxies at low redshift, with...
Studying the build-up of mass and angular momentum in galaxies is fundamental to understanding the l...
We investigate the relationship between stellar and gas specific angular momentum j, stellar mass M⁎...
We investigate the relationship between stellar and gas specific angular momentum j, stellar massM* ...
Aims. At intermediate redshift, galaxy groups and clusters are thought to impact galaxy properties s...
Aims. At intermediate redshift, galaxy groups and clusters are thought to impact galaxy properties s...
We study the spatially resolved stellar specific angular momentum j* in a high-quality sample of 24 ...
We measure λRe, a proxy for galaxy specific stellar angular momentum within one effective radius, an...
We measure λRe, a proxy for galaxy specific stellar angular momentum within one effective radius, an...
Context. Galaxy formation in the current cosmological paradigm is a very complex process in which in...
Angular momentum (AM) is a key parameter to understand galaxy formation and evolution. AM originates...
Galaxy formation is a very complex process in which many different physical mechanisms intervene. Wi...
We investigate the stellar angular momentum of galaxies across the Hubble sequence from the CALIFA s...
We study 379 central and 159 satellite early-type galaxies with two-dimensional kinematics from the ...
The “kinematic” morphology–density relation for early-type galaxies posits that those galaxies with ...