Add to ORKGAcceptedInternational audienceContext. Classical Be stars are hot non-supergiant stars surrounded by...
Context. Herbig Ae/Be stars (HAeBes) have so far been studied based on relatively small samples that...
Optical long baseline interferometry was recently established as a technique capable of resolving st...
As estrelas Be compreendem uma grande faixa de massas e temperaturas. Por definição, são objetos de ...
This thesis presents a spectroscopic study of the stellar properties, accretion rates, and emission ...
Classical Be stars are the only Main Sequence stars that possess Keplerian decretion circumstellar d...
Using the photometric and Be-star catalogues existing at La Plata, the photometric behavior of a sam...
As estrelas Herbig Ae/Be (HAeBe) representam os objetos de massa intermediária (2-10 Msol) na pré-se...
The circumstellar disks ejected by many rapidly rotating B stars (so-called Be stars) offer the rare...
The general objective of the present work is to contribute to the knowledge of the physics of Be Sta...
A espectrocopia de estrelas Be realizada com alta resolução e alta relação sinal/ruído permite inves...
Aims.We investigate evidence of accretion in a sample of 15 Herbig Ae/Be stars to determine whether ...
Herbig Ae/Be stars are pre-main sequence sources, canonically defined as having masses 2 Msun < M < ...
The definition of Be stars (Jaschek et al. 1981) as non-supergiant B stars which at least once have ...
The main objective of this PhD thesis was to add new elements to the knowledge of hot active stars a...
AcceptedInternational audienceContext. Classical Be stars are hot non-supergiant stars surrounded by...
Context. Herbig Ae/Be stars (HAeBes) have so far been studied based on relatively small samples that...
Optical long baseline interferometry was recently established as a technique capable of resolving st...
As estrelas Be compreendem uma grande faixa de massas e temperaturas. Por definição, são objetos de ...
This thesis presents a spectroscopic study of the stellar properties, accretion rates, and emission ...
Classical Be stars are the only Main Sequence stars that possess Keplerian decretion circumstellar d...
Using the photometric and Be-star catalogues existing at La Plata, the photometric behavior of a sam...
As estrelas Herbig Ae/Be (HAeBe) representam os objetos de massa intermediária (2-10 Msol) na pré-se...
The circumstellar disks ejected by many rapidly rotating B stars (so-called Be stars) offer the rare...
The general objective of the present work is to contribute to the knowledge of the physics of Be Sta...
A espectrocopia de estrelas Be realizada com alta resolução e alta relação sinal/ruído permite inves...
Aims.We investigate evidence of accretion in a sample of 15 Herbig Ae/Be stars to determine whether ...
Herbig Ae/Be stars are pre-main sequence sources, canonically defined as having masses 2 Msun < M < ...
The definition of Be stars (Jaschek et al. 1981) as non-supergiant B stars which at least once have ...
The main objective of this PhD thesis was to add new elements to the knowledge of hot active stars a...
AcceptedInternational audienceContext. Classical Be stars are hot non-supergiant stars surrounded by...
Context. Herbig Ae/Be stars (HAeBes) have so far been studied based on relatively small samples that...
Optical long baseline interferometry was recently established as a technique capable of resolving st...