Context. The diffuse ionized gas (DIG) constitutes the largest fraction of the total ionized interstellar matter in star-forming galaxies, but it is still unclear whether the ionization is driven predominantly by the ionizing radiation of hot massive stars, as in H I
I review the properties of the di#use ionized gas (DIG) in nearby star-forming galaxies emphasizing ...
International audienceWe revisit the question of the ionization of the diffuse medium in late-type g...
International audienceWe revisit the question of the ionization of the diffuse medium in late-type g...
The diffuse ionized gas (DIG) is an important component of the interstellar medium (ISM), and it can...
International audienceWe use integral field spectroscopy from the PHANGS-MUSE survey, which resolves...
International audienceWe use integral field spectroscopy from the PHANGS-MUSE survey, which resolves...
We demonstrate that the observed increase of some nebular line ratios with height above the midplane...
Aims. The aim of this work is to verify whether turbulent magnetic reconnection can provide the addi...
The Diffuse Ionized Gas (DIG) contributes to the nebular emission of galaxies, resulting in emission...
The diffuse ionized gas (DIG) in galaxies traces photoionization feedback from massive stars. Throug...
The diffuse ionized gas (DIG) in galaxies traces photoionization feedback from massive stars. Throug...
Diffuse ionized gas (DIG) is prevalent in star-forming galaxies. Using a sample of 365 nearly face-o...
Diffuse ionized gas (DIG) is prevalent in star-forming galaxies. Using a sample of 365 nearly face-o...
Diese Doktorarbeit beschäftigt sich mit der Modellierung des Diffus Ionisierten Gases (DIG) in unser...
Diffuse ionized gas (DIG) is prevalent in star-forming galaxies. Using a sample of 365 nearly face-o...
I review the properties of the di#use ionized gas (DIG) in nearby star-forming galaxies emphasizing ...
International audienceWe revisit the question of the ionization of the diffuse medium in late-type g...
International audienceWe revisit the question of the ionization of the diffuse medium in late-type g...
The diffuse ionized gas (DIG) is an important component of the interstellar medium (ISM), and it can...
International audienceWe use integral field spectroscopy from the PHANGS-MUSE survey, which resolves...
International audienceWe use integral field spectroscopy from the PHANGS-MUSE survey, which resolves...
We demonstrate that the observed increase of some nebular line ratios with height above the midplane...
Aims. The aim of this work is to verify whether turbulent magnetic reconnection can provide the addi...
The Diffuse Ionized Gas (DIG) contributes to the nebular emission of galaxies, resulting in emission...
The diffuse ionized gas (DIG) in galaxies traces photoionization feedback from massive stars. Throug...
The diffuse ionized gas (DIG) in galaxies traces photoionization feedback from massive stars. Throug...
Diffuse ionized gas (DIG) is prevalent in star-forming galaxies. Using a sample of 365 nearly face-o...
Diffuse ionized gas (DIG) is prevalent in star-forming galaxies. Using a sample of 365 nearly face-o...
Diese Doktorarbeit beschäftigt sich mit der Modellierung des Diffus Ionisierten Gases (DIG) in unser...
Diffuse ionized gas (DIG) is prevalent in star-forming galaxies. Using a sample of 365 nearly face-o...
I review the properties of the di#use ionized gas (DIG) in nearby star-forming galaxies emphasizing ...
International audienceWe revisit the question of the ionization of the diffuse medium in late-type g...
International audienceWe revisit the question of the ionization of the diffuse medium in late-type g...