Add to ORKGInternational audienceWe present a quantitative study of massive stars in the High Excitation Blob N81, a compact star forming region in the SMC. The stellar content was resolved by HST, and STIS was used to obtain medium resolution spectra. The qualitative analysis of the stellar properties presented in Heydari-Malayeri et al. (\cite{papI}) is extended using non-LTE spherically extended atmosphere models including line-blanketing computed with the code CMFGEN (Hillier & Miller \cite{hm98}), and the wind properties are investigated. The main results are the following
[Abridged] We present high-resolution optical HST/STIS observations made with two slits crossing fou...
[Abridged] We have studied the optical spectra of 28 O- and early B-type stars in the Large Magellan...
We examine the feasibility of using medium resolution spectra for determining the parameters of the ...
International audienceWe present a quantitative study of massive stars in the High Excitation Blob N...
Using Hubble Space Telescope observations with STIS, we study the main exciting stars of N81, a high...
International audienceContext: How star formation proceeds in the Galactic Center is a debated quest...
In this paper we review the observational data for OB stars in the SMC concentrating on those aspect...
We present near infrared JHK imaging of the Small Magellanic Cloud compact $\ion{H}{ii}$ region N81...
Context. The star cluster R136 inside the Large Magellanic Cloud hosts a rich population of massive ...
[Abridged] We present high-resolution optical HST/STIS observations made with two slits crossing fou...
[Abridged] We have studied the optical spectra of 28 O- and early B-type stars in the Large Magellan...
We examine the feasibility of using medium resolution spectra for determining the parameters of the ...
International audienceWe present a quantitative study of massive stars in the High Excitation Blob N...
Using Hubble Space Telescope observations with STIS, we study the main exciting stars of N81, a high...
International audienceContext: How star formation proceeds in the Galactic Center is a debated quest...
In this paper we review the observational data for OB stars in the SMC concentrating on those aspect...
We present near infrared JHK imaging of the Small Magellanic Cloud compact $\ion{H}{ii}$ region N81...
Context. The star cluster R136 inside the Large Magellanic Cloud hosts a rich population of massive ...
[Abridged] We present high-resolution optical HST/STIS observations made with two slits crossing fou...
[Abridged] We have studied the optical spectra of 28 O- and early B-type stars in the Large Magellan...
We examine the feasibility of using medium resolution spectra for determining the parameters of the ...