Interstellar bubbles around O stars are driven by a combination of the star’s wind and ionizing radiation output. The wind contribution is uncertain because the boundary between the wind and interstellar medium is difficult to observe. Mid-infrared observations (e.g., of the H i
Context. The [CII] 158 mu m fine-structure line is one of the dominant coolants of the neutral inter...
A visual examination of the images from the Galactic Legacy Infrared Mid-Plane Survey Extraordinaire...
Context. OB-type stars have strong ionizing radiation and drive energetic winds. The ultraviolet rad...
Interstellar bubbles around O stars are driven by a combination of the star’s wind and ionizing radi...
Mid-infrared arcs of dust emission are often seen near ionizing stars within H i
Massive stars drive the evolution of the interstellar medium through their radiative and mechanical ...
Context. Interstellar bubbles are structures in the interstellar medium with diameters of ...
Abstract. We study the dynamics of stellar wind bubbles around hydrogen-deficient stars using numeri...
Author manuscript version. The final article is available online from the publisher via: http://d...
International audienceContext. The interstellar bubble RCW 120 seen around a type O runaway star is ...
We study the dynamics of stellar wind bubbles around hydrogen-deficient stars using numerical simul...
Context. The Orion Molecular Cloud is the nearest massive-star forming region. Massive stars have pr...
Stellar winds from O and WR stars transfer large amounts of mechanical energy and momentum into the ...
The Bubble Nebula (or NGC 7635) is a parsec-scale seemingly spherical wind-blown bubble around the r...
We have examined the interstellar medium in the vicinity of massive stars belonging to the Per OB1 a...
Context. The [CII] 158 mu m fine-structure line is one of the dominant coolants of the neutral inter...
A visual examination of the images from the Galactic Legacy Infrared Mid-Plane Survey Extraordinaire...
Context. OB-type stars have strong ionizing radiation and drive energetic winds. The ultraviolet rad...
Interstellar bubbles around O stars are driven by a combination of the star’s wind and ionizing radi...
Mid-infrared arcs of dust emission are often seen near ionizing stars within H i
Massive stars drive the evolution of the interstellar medium through their radiative and mechanical ...
Context. Interstellar bubbles are structures in the interstellar medium with diameters of ...
Abstract. We study the dynamics of stellar wind bubbles around hydrogen-deficient stars using numeri...
Author manuscript version. The final article is available online from the publisher via: http://d...
International audienceContext. The interstellar bubble RCW 120 seen around a type O runaway star is ...
We study the dynamics of stellar wind bubbles around hydrogen-deficient stars using numerical simul...
Context. The Orion Molecular Cloud is the nearest massive-star forming region. Massive stars have pr...
Stellar winds from O and WR stars transfer large amounts of mechanical energy and momentum into the ...
The Bubble Nebula (or NGC 7635) is a parsec-scale seemingly spherical wind-blown bubble around the r...
We have examined the interstellar medium in the vicinity of massive stars belonging to the Per OB1 a...
Context. The [CII] 158 mu m fine-structure line is one of the dominant coolants of the neutral inter...
A visual examination of the images from the Galactic Legacy Infrared Mid-Plane Survey Extraordinaire...
Context. OB-type stars have strong ionizing radiation and drive energetic winds. The ultraviolet rad...
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