Mid-infrared arcs of dust emission are often seen near ionizing stars within H i
International audienceBecause of their relatively simple morphology, "bubble" HII regions have been ...
Context. Hot exozodiacal dust has been shown to be present in the innermost regions of an increasing...
Context. The [CII] 158 mu m fine-structure line is one of the dominant coolants of the neutral inter...
Mid-infrared arcs of dust emission are often seen near ionizing stars within H i
Interstellar bubbles around O stars are driven by a combination of the star’s wind and ionizing radi...
Author manuscript version. The final article is available online from the publisher via: http://d...
Context. Hot exozodiacal dust has been shown to be present in the innermost regions of an increasing...
International audienceContext. Hot exozodiacal dust has been shown to be present in the innermost re...
We present new observations of the near-infrared hydrogen recombination lines Paβ and Bry in the cen...
Context. The infrared emission (IR) of the interstellar dust has been claimed to be a tracer of the ...
Aims. We investigate the environment of the infrared dust bubble S51 and search for evidence of trig...
The physical mechanisms that induce the transformation of a certain mass of gas in new stars are far...
ABSTRACT. The luminosity of the central source in ionizing radiation is an essential parameter in a ...
We report observations of diffuse far‐infrared emission from interstellar dust at high Galactic lati...
International audienceBecause of their relatively simple morphology, "bubble" HII regions have been ...
Context. Hot exozodiacal dust has been shown to be present in the innermost regions of an increasing...
Context. The [CII] 158 mu m fine-structure line is one of the dominant coolants of the neutral inter...
Mid-infrared arcs of dust emission are often seen near ionizing stars within H i
Interstellar bubbles around O stars are driven by a combination of the star’s wind and ionizing radi...
Author manuscript version. The final article is available online from the publisher via: http://d...
Context. Hot exozodiacal dust has been shown to be present in the innermost regions of an increasing...
International audienceContext. Hot exozodiacal dust has been shown to be present in the innermost re...
We present new observations of the near-infrared hydrogen recombination lines Paβ and Bry in the cen...
Context. The infrared emission (IR) of the interstellar dust has been claimed to be a tracer of the ...
Aims. We investigate the environment of the infrared dust bubble S51 and search for evidence of trig...
The physical mechanisms that induce the transformation of a certain mass of gas in new stars are far...
ABSTRACT. The luminosity of the central source in ionizing radiation is an essential parameter in a ...
We report observations of diffuse far‐infrared emission from interstellar dust at high Galactic lati...
International audienceBecause of their relatively simple morphology, "bubble" HII regions have been ...
Context. Hot exozodiacal dust has been shown to be present in the innermost regions of an increasing...
Context. The [CII] 158 mu m fine-structure line is one of the dominant coolants of the neutral inter...