IAR   05382
INSTITUTO ARGENTINO DE RADIOASTRONOMIA
Unidad Ejecutora - UE
congresos y reuniones científicas
Título:
Gamma-rays from star forming regions
Autor/es:
G. E. ROMERO
Lugar:
Heidelberg, Alemania
Reunión:
Simposio; High Energy Gamma-ray Astronomy; 2008
Resumen:
Abstract. Star-forming regions have been tentatively associated with gamma-ray sources since the early days of the COS
B satellite. After the Compton Gamma-Ray Observatory, the statistical evidence for such an association has became
overwhelming. Recent results from Cherenkov telescopes indicate that some high-energy sources are produced in regions
of active star formation like Cygnus OB2 and Westerlund 2. In this paper I will briefly review what kind of stellar objects can
produce gamma-ray emission in star-forming regions and I will suggest that the formation process of massive stars could in
principle result in the production of observable gamma rays
B satellite. After the Compton Gamma-Ray Observatory, the statistical evidence for such an association has became
overwhelming. Recent results from Cherenkov telescopes indicate that some high-energy sources are produced in regions
of active star formation like Cygnus OB2 and Westerlund 2. In this paper I will briefly review what kind of stellar objects can
produce gamma-ray emission in star-forming regions and I will suggest that the formation process of massive stars could in
principle result in the production of observable gamma rays
B satellite. After the Compton Gamma-Ray Observatory, the statistical evidence for such an association has became
overwhelming. Recent results from Cherenkov telescopes indicate that some high-energy sources are produced in regions
of active star formation like Cygnus OB2 and Westerlund 2. In this paper I will briefly review what kind of stellar objects can
produce gamma-ray emission in star-forming regions and I will suggest that the formation process of massive stars could in
principle result in the production of observable gamma rays
Star-forming regions have been tentatively associated with gamma-ray sources since the early days of the COS
B satellite. After the Compton Gamma-Ray Observatory, the statistical evidence for such an association has became
overwhelming. Recent results from Cherenkov telescopes indicate that some high-energy sources are produced in regions
of active star formation like Cygnus OB2 and Westerlund 2. In this paper I will briefly review what kind of stellar objects can
produce gamma-ray emission in star-forming regions and I will suggest that the formation process of massive stars could in
principle result in the production of observable gamma rays