Add to ORKGWe report the case of the geometrical and kinematical decoupling between the bulge and the disk of the Sa galaxy NGC 4698. The R-band isophotal map of this spiral shows that the bulge structure is elongated perpendicularly to the major axis of the disk. At the same time a central stellar velocity gradient is found along the major axis of the bulge. We also present the Sa NGC 4672 as good candidate of a spiral hosting a bulge and a disk orthogonally decoupled with respect to one other. This decoupling of the two fundamental components of a visible galaxy suggests that the disk could represent a second event in the history of early-type spirals
Kinematic and population studies show that bulges are generally rotationally flattened systems simil...
We present major and minor-axis kinematics of stars and ionized gas as well as narrow and broad-band...
We report evidence for nuclear stellar disks in three early-type spirals, namely, NGC 1425, NGC 3898...
The R-band isophotal map of the Sa galaxy NGC 4698 shows that the inner region of the bulge is elong...
The R-band isophotal map of the Sa galaxy NGC 4698 shows that the inner region of the bulge structur...
We report the case of the geometrical and kinematical decoupling between the bulge and the disk of t...
We report the case of the early-type disk galaxy NGC 4672 as a new example of a galaxy hosting a bul...
The R-band isophotal map of the Sa galaxy NGC 4698 shows that the inner region of the bulge structur...
Like fossils, multiple stellar and gaseous components with a misaligned or even opposite angular mom...
We report the case of the early-type disk galaxy NGC 4672 as a new example of a galaxy characterized...
Kinematical decoupling between two components of a galaxy suggests the occurrence of a second event....
The early-type spiral NGC 4698 is known to host a nuclear disc of gas and stars which is rotating pe...
The morphological features of the early-type disk galaxy NGC 4672 are discussed as well as the veloc...
We present detailed morphological, photometric, and stellar-kinematic analyses of the central region...
We report evidence for nuclear stellar disks in three early-type spirals, namely, NGC 1425, NGC 3898...
Kinematic and population studies show that bulges are generally rotationally flattened systems simil...
We present major and minor-axis kinematics of stars and ionized gas as well as narrow and broad-band...
We report evidence for nuclear stellar disks in three early-type spirals, namely, NGC 1425, NGC 3898...
The R-band isophotal map of the Sa galaxy NGC 4698 shows that the inner region of the bulge is elong...
The R-band isophotal map of the Sa galaxy NGC 4698 shows that the inner region of the bulge structur...
We report the case of the geometrical and kinematical decoupling between the bulge and the disk of t...
We report the case of the early-type disk galaxy NGC 4672 as a new example of a galaxy hosting a bul...
The R-band isophotal map of the Sa galaxy NGC 4698 shows that the inner region of the bulge structur...
Like fossils, multiple stellar and gaseous components with a misaligned or even opposite angular mom...
We report the case of the early-type disk galaxy NGC 4672 as a new example of a galaxy characterized...
Kinematical decoupling between two components of a galaxy suggests the occurrence of a second event....
The early-type spiral NGC 4698 is known to host a nuclear disc of gas and stars which is rotating pe...
The morphological features of the early-type disk galaxy NGC 4672 are discussed as well as the veloc...
We present detailed morphological, photometric, and stellar-kinematic analyses of the central region...
We report evidence for nuclear stellar disks in three early-type spirals, namely, NGC 1425, NGC 3898...
Kinematic and population studies show that bulges are generally rotationally flattened systems simil...
We present major and minor-axis kinematics of stars and ionized gas as well as narrow and broad-band...
We report evidence for nuclear stellar disks in three early-type spirals, namely, NGC 1425, NGC 3898...