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The circumgalactic medium
The gas surrounding galaxies outside their disks or interstellar medium and inside their virial
radii is known as the circumgalactic medium (CGM). In recent years this component of …
radii is known as the circumgalactic medium (CGM). In recent years this component of …
Structure and kinematics of early-type galaxies from integral field spectroscopy
Observations of galaxy isophotes, long-slit kinematics, and high-resolution photometry
suggested a possible dichotomy between two distinct classes of elliptical galaxies. But these …
suggested a possible dichotomy between two distinct classes of elliptical galaxies. But these …
JADES: Insights into the low-mass end of the mass–metallicity–SFR relation at 3< z< 10 from deep JWST/NIRSpec spectroscopy
We analysed the gas-phase metallicity properties of a sample of low-stellar-mass (log
M⋆/M⊙≲ 9) galaxies at 3< z< 10 observed with JWST/NIRSpec as part of the JADES …
M⋆/M⊙≲ 9) galaxies at 3< z< 10 observed with JWST/NIRSpec as part of the JADES …
The Dawes Review 9: The role of cold gas strip** on the star formation quenching of satellite galaxies
One of the key open questions in extragalactic astronomy is what stops star formation in
galaxies. While it is clear that the cold gas reservoir, which fuels the formation of new stars …
galaxies. While it is clear that the cold gas reservoir, which fuels the formation of new stars …
SDSS IV MaNGA–metallicity and nitrogen abundance gradients in local galaxies
We study the gas phase metallicity (O/H) and nitrogen abundance gradients traced by star-
forming regions in a representative sample of 550 nearby galaxies in the stellar mass range …
forming regions in a representative sample of 550 nearby galaxies in the stellar mass range …
Gaseous galaxy halos
Galactic halo gas traces inflowing star-formation fuel and feedback from a galaxy's disk and
is therefore crucial to our understanding of galaxy evolution. In this review, we summarize …
is therefore crucial to our understanding of galaxy evolution. In this review, we summarize …
How cold gas continuously entrains mass and momentum from a hot wind
The existence of fast moving, cold gas ubiquitously observed in galactic winds is
theoretically puzzling, since the destruction time of cold gas is much smaller than its …
theoretically puzzling, since the destruction time of cold gas is much smaller than its …
Numerical simulations of multiphase winds and fountains from star-forming galactic disks. I. Solar neighborhood TIGRESS model
Gas blown away from galactic disks by supernova (SN) feedback plays a key role in galaxy
evolution. We investigate outflows utilizing the solar neighborhood model of our high …
evolution. We investigate outflows utilizing the solar neighborhood model of our high …
Chemical evolution with radial mixing
R Schönrich, J Binney - Monthly Notices of the Royal …, 2009 - academic.oup.com
Abstract Models of the chemical evolution of our Galaxy are extended to include radial
migration of stars and flow of gas through the disc. The models track the production of both …
migration of stars and flow of gas through the disc. The models track the production of both …
Cold gas accretion in galaxies
Evidence for the accretion of cold gas in galaxies has been rapidly accumulating in the past
years. HI observations of galaxies and their environment have brought to light new facts and …
years. HI observations of galaxies and their environment have brought to light new facts and …