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 present the SAMI Pilot Survey, consisting of integral field spectroscopy of 106 galaxies across t...
The “kinematic” morphology–density relation for early-type galaxies posits that those galaxies with ...
Motivated by a new wave of kinematical tracers in the outer regions of early-type galaxies (elliptic...
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 massM* ...
The kinematic morphology–density relation for early-type galaxies posits that those galaxies with ...
We investigate the relationship between stellar and gas specific angular momentum j, stellar mass M⁎...
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...
The angular momentum of galaxies controls the kinematics of their stars, which in turn drives observ...
We measure λRe, a proxy for galaxy specific stellar angular momentum within one effective radius, a...
We present a MUSE and KMOS dynamical study 405 star-forming galaxies at redshift z=0.28-1.65 (median...
International audienceWe present a MUSE (Multi‐Unit Spectroscopic Explorer) and KMOS (K‐band Multi‐O...
Context. Galaxy formation in the current cosmological paradigm is a verycomplex process in which inf...
We present the SAMI Pilot Survey, consisting of integral field spectroscopy of 106 galaxies across t...
The “kinematic” morphology–density relation for early-type galaxies posits that those galaxies with ...
Motivated by a new wave of kinematical tracers in the outer regions of early-type galaxies (elliptic...
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 massM* ...
The kinematic morphology–density relation for early-type galaxies posits that those galaxies with ...
We investigate the relationship between stellar and gas specific angular momentum j, stellar mass M⁎...
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...
The angular momentum of galaxies controls the kinematics of their stars, which in turn drives observ...
We measure λRe, a proxy for galaxy specific stellar angular momentum within one effective radius, a...
We present a MUSE and KMOS dynamical study 405 star-forming galaxies at redshift z=0.28-1.65 (median...
International audienceWe present a MUSE (Multi‐Unit Spectroscopic Explorer) and KMOS (K‐band Multi‐O...
Context. Galaxy formation in the current cosmological paradigm is a verycomplex process in which inf...
We present the SAMI Pilot Survey, consisting of integral field spectroscopy of 106 galaxies across t...
The “kinematic” morphology–density relation for early-type galaxies posits that those galaxies with ...
Motivated by a new wave of kinematical tracers in the outer regions of early-type galaxies (elliptic...