Context. Recently it has been found that models of massive stars reach the Eddington limit in their interior, which leads to dilute extended envelopes
One of the key questions in Astrophysics concerns the issue of whether there exists an upper-mass li...
In addition to being spectacular objects, Very Massive Stars (VMS) are suspected to have a tremendou...
We conduct a theoretical study of the formation of massive stars over a wide range of metallicities ...
Context. Massive stars play a vital role in the Universe, however, their evolution even on the main-...
Context. Massive stars play a vital role in the Universe, however, their evolution even on the main-...
Context. Massive stars play a vital role in the Universe, however, their evolution even on the main-...
Context. Massive stars play a vital role in the Universe, however, their evolution even on the main-...
Context. It has been proposed that the envelopes of luminous stars may be subject to substantial rad...
Context. It has been proposed that the envelopes of luminous stars may be subject to substantial rad...
Context. The proximity to the Eddington luminosity has been attributed as the cause of several obser...
Context. The proximity to the Eddington luminosity has been attributed as the cause of several obser...
The proximity to the Eddington luminosity has been attributed as the cause of several observed effec...
Metallicity is known to significantly affect the radial expansion of a massive star: the lower the m...
We have determined the location of the line-opacity modified Eddington limit for stars in the LMC us...
One of the key questions in Astrophysics concerns the issue of whether there exists an upper-mass li...
One of the key questions in Astrophysics concerns the issue of whether there exists an upper-mass li...
In addition to being spectacular objects, Very Massive Stars (VMS) are suspected to have a tremendou...
We conduct a theoretical study of the formation of massive stars over a wide range of metallicities ...
Context. Massive stars play a vital role in the Universe, however, their evolution even on the main-...
Context. Massive stars play a vital role in the Universe, however, their evolution even on the main-...
Context. Massive stars play a vital role in the Universe, however, their evolution even on the main-...
Context. Massive stars play a vital role in the Universe, however, their evolution even on the main-...
Context. It has been proposed that the envelopes of luminous stars may be subject to substantial rad...
Context. It has been proposed that the envelopes of luminous stars may be subject to substantial rad...
Context. The proximity to the Eddington luminosity has been attributed as the cause of several obser...
Context. The proximity to the Eddington luminosity has been attributed as the cause of several obser...
The proximity to the Eddington luminosity has been attributed as the cause of several observed effec...
Metallicity is known to significantly affect the radial expansion of a massive star: the lower the m...
We have determined the location of the line-opacity modified Eddington limit for stars in the LMC us...
One of the key questions in Astrophysics concerns the issue of whether there exists an upper-mass li...
One of the key questions in Astrophysics concerns the issue of whether there exists an upper-mass li...
In addition to being spectacular objects, Very Massive Stars (VMS) are suspected to have a tremendou...
We conduct a theoretical study of the formation of massive stars over a wide range of metallicities ...
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