SAMI Galaxy Survey: gas streaming

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Line-of-sight velocities of gas and stars can constrain dark matter (DM) within rotationally supported galaxies if they trace circular orbits extensively. Photometric...

SAMI Galaxy Survey: gas streaming

VizieR online Data Catalogue associated with article published in journal Monthly Notices of the Royal Astronomical Society with title ' The SAMI Galaxy Survey: gas streaming and dynamical M/L in rota

DataCite Commons2024-08-17 更新130

Data from : The SAMI Galaxy Survey: stellar and gas misalignments and the origin of gas in nearby galaxies

Misalignment of gas and stellar rotation in galaxies can give clues to the origin and processing of accreted gas. Integral field spectroscopic observations of 1213 galaxies from the Sydney-AAO Multi-o

Research Data Australia50

SAMI Galaxy Survey asymmetries

We study the properties of kinematically disturbed galaxies in the Sydney-AAO Multi-object Integral field spectrograph (SAMI) Galaxy Survey using a quantitative criterion, based...

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SAMI Galaxy Survey. Gas surface densities

VizieR online Data Catalogue associated with article published in journal Monthly Notices of the Royal Astronomical Society with title ' The SAMI Galaxy Survey: a new method to estimate molecular gas

DataCite Commons2024-08-17 更新100

SAMI Galaxy Survey. Gas surface densities

Stars form in cold molecular clouds. However, molecular gas is difficult to observe because the most abundant molecule (H_2_) lacks a permanent dipole moment. Rotational...

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