Add to ORKGWe analyze asymmetries in the gas rotation curves of 113 galaxies drawn from the Nearby Field Galaxy Survey, spanning a broad range of luminosities and morphologies. If the origin of the rotation curve is chosen to minimize the asymmetry, then ~23% of sample galaxies show asymmetry >5% within 1.3r_e. However, not all gas kinematic asymmetries indicate asymmetries in the underlying potential
Morphological asymmetries between the approaching and receding sides in both the stellar and neutral...
Galaxy rotation has been studied for over a century, using spectroscopic measurements to construct r...
We are determining rotation curves for the galaxies in the RESOLVE (REsolved Spectroscopy Of a Local...
Asymmetries in the distribution of light and neutral hydrogen are often observed in spiral galaxies....
Many spiral galaxies show a large-scale asymmetry with a cos φ dependence in their rotation...
We present a detailed study of rotational asymmetry in galaxies for both morphological and physical ...
We present a detailed study of rotational asymmetry in galaxies for both morphological and physical ...
We use Gaia-TGAS data to compare the transverse velocities in Galactic longitude (coming from proper...
Many spiral galaxies show a large-scale asymmetry with a cos\phi dependence in their rotation curves...
The frequently observed lopsidedness of the distribution of stars and gas in disc galaxies is still ...
We study the properties of kinematically disturbed galaxies in the Sydney-AAO Multi-object Integral ...
We study the properties of kinematically disturbed galaxies in the Sydney-AAO Multi-object Integral ...
We study the properties of kinematically disturbed galaxies in the Sydney-AAO Multi-object Integral ...
Asymmetries in the distributions of light and neutral hydrogen are often observed in disk galaxies. ...
Morphological asymmetries between the approaching and receding sides in both the stellar and neutral...
Galaxy rotation has been studied for over a century, using spectroscopic measurements to construct r...
We are determining rotation curves for the galaxies in the RESOLVE (REsolved Spectroscopy Of a Local...
Asymmetries in the distribution of light and neutral hydrogen are often observed in spiral galaxies....
Many spiral galaxies show a large-scale asymmetry with a cos φ dependence in their rotation...
We present a detailed study of rotational asymmetry in galaxies for both morphological and physical ...
We present a detailed study of rotational asymmetry in galaxies for both morphological and physical ...
We use Gaia-TGAS data to compare the transverse velocities in Galactic longitude (coming from proper...
Many spiral galaxies show a large-scale asymmetry with a cos\phi dependence in their rotation curves...
The frequently observed lopsidedness of the distribution of stars and gas in disc galaxies is still ...
We study the properties of kinematically disturbed galaxies in the Sydney-AAO Multi-object Integral ...
We study the properties of kinematically disturbed galaxies in the Sydney-AAO Multi-object Integral ...
We study the properties of kinematically disturbed galaxies in the Sydney-AAO Multi-object Integral ...
Asymmetries in the distributions of light and neutral hydrogen are often observed in disk galaxies. ...
Morphological asymmetries between the approaching and receding sides in both the stellar and neutral...
Galaxy rotation has been studied for over a century, using spectroscopic measurements to construct r...
We are determining rotation curves for the galaxies in the RESOLVE (REsolved Spectroscopy Of a Local...