We critically examine a scenario for the enrichment of the interstellar medium (ISM) in which supernova ejecta follow a long (108 yr) journey before falling back onto the galactic disk in the form of metal-rich “droplets”, These droplets do not become fully mixed with the interstellar medium until they become photoionized in H i
7 pages, 3 figures, ASTRO2020 white paperThe comparison of chemical abundances in the neutral gas of...
Whereas the extreme conditions of the first minutes after the Big Bang have prod...
none3noWe investigate the impact of supernova (SN) feedback in gas-rich dwarf galaxies experiencing ...
International audienceWe critically examine a scenario for the enrichment of the interstellar medium...
Observations give evidences of the presence of metals in the intergalactic medium (IGM). The stars r...
The abundance evolution of galaxies depends critically on the balance between the mix-ing of metals ...
International audienceThe Interstellar Medium (ISM) comprises gases at different temperatures and de...
The term “Milky Way” usually refers to the hundreds billion stars of our Galaxy, which emit most of ...
Using the Eris zoom-in cosmological simulation of assembly of a Milky Way analogue, we study the che...
With the installation of the Cosmic Origins Spectrograph on the Hubble Space Telescope, measurements...
As building blocks of dust, rocky planets, and even complex life, the chemical elements heavier than...
Observations have established that the diffuse intergalactic medium (IGM) at z ~ 3 is enriched to ~1...
We assess supernova (SN)-driven pregalactic outflows as a mechanism for distributing the product of ...
Context. The presence of dust in the neutral interstellar medium (ISM) dramatically changes the meta...
264 p.Thesis (Ph.D.)--University of Illinois at Urbana-Champaign, 2005.In the second part of this wo...
7 pages, 3 figures, ASTRO2020 white paperThe comparison of chemical abundances in the neutral gas of...
Whereas the extreme conditions of the first minutes after the Big Bang have prod...
none3noWe investigate the impact of supernova (SN) feedback in gas-rich dwarf galaxies experiencing ...
International audienceWe critically examine a scenario for the enrichment of the interstellar medium...
Observations give evidences of the presence of metals in the intergalactic medium (IGM). The stars r...
The abundance evolution of galaxies depends critically on the balance between the mix-ing of metals ...
International audienceThe Interstellar Medium (ISM) comprises gases at different temperatures and de...
The term “Milky Way” usually refers to the hundreds billion stars of our Galaxy, which emit most of ...
Using the Eris zoom-in cosmological simulation of assembly of a Milky Way analogue, we study the che...
With the installation of the Cosmic Origins Spectrograph on the Hubble Space Telescope, measurements...
As building blocks of dust, rocky planets, and even complex life, the chemical elements heavier than...
Observations have established that the diffuse intergalactic medium (IGM) at z ~ 3 is enriched to ~1...
We assess supernova (SN)-driven pregalactic outflows as a mechanism for distributing the product of ...
Context. The presence of dust in the neutral interstellar medium (ISM) dramatically changes the meta...
264 p.Thesis (Ph.D.)--University of Illinois at Urbana-Champaign, 2005.In the second part of this wo...
7 pages, 3 figures, ASTRO2020 white paperThe comparison of chemical abundances in the neutral gas of...
Whereas the extreme conditions of the first minutes after the Big Bang have prod...
none3noWe investigate the impact of supernova (SN) feedback in gas-rich dwarf galaxies experiencing ...
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