Add to ORKGHigh-energy radiation and particles profoundly affect circumstellar disk gas and solids. We discuss stellar high-energy sources and summarize their effects on circumstellar disk
We report the detection of [Ne II] emission at 12.81 μm in four out of the six optically thick dust ...
There is now a substantial body of evidence that disk-like structures of gas and dust surround many ...
Context. Anomalies in the abundance measurements of short lived radionuclides in meteorites indicate...
The early solar system represents the only case we have of a circumstellar disk that can be investig...
Nearby, young stars are the ideal targets for investigations of stellar and protoplanetary disk evol...
High-energy radiation from the central T Tauri and protostars plays an important role in shaping pro...
Anomalies in the abundance measurements of short lived radionuclides in meteorites indicate that the...
Young stars are well known for being strong X-ray emitters. This emission can be originated by diffe...
Accretion disks around young stars produce excess infrared continuum associated with the disk and ex...
The research leading to these results has received funding from the European Union Seventh Framework...
According to the magnetospheric accretion scenario, young low-mass stars are surrounded by circumste...
A hot, two-temperature accretion disk can be a strong γ-ray and relativistic particle source. This o...
We present new X-ray and far-ultraviolet (FUV) observations of T Tauri stars covering the age range ...
We assess the ionizing effect of low-energy protostellar cosmic rays in protoplanetary discs around...
Although the environments of star and planet formation are thermodynamically cold, substantial X-ray...
We report the detection of [Ne II] emission at 12.81 μm in four out of the six optically thick dust ...
There is now a substantial body of evidence that disk-like structures of gas and dust surround many ...
Context. Anomalies in the abundance measurements of short lived radionuclides in meteorites indicate...
The early solar system represents the only case we have of a circumstellar disk that can be investig...
Nearby, young stars are the ideal targets for investigations of stellar and protoplanetary disk evol...
High-energy radiation from the central T Tauri and protostars plays an important role in shaping pro...
Anomalies in the abundance measurements of short lived radionuclides in meteorites indicate that the...
Young stars are well known for being strong X-ray emitters. This emission can be originated by diffe...
Accretion disks around young stars produce excess infrared continuum associated with the disk and ex...
The research leading to these results has received funding from the European Union Seventh Framework...
According to the magnetospheric accretion scenario, young low-mass stars are surrounded by circumste...
A hot, two-temperature accretion disk can be a strong γ-ray and relativistic particle source. This o...
We present new X-ray and far-ultraviolet (FUV) observations of T Tauri stars covering the age range ...
We assess the ionizing effect of low-energy protostellar cosmic rays in protoplanetary discs around...
Although the environments of star and planet formation are thermodynamically cold, substantial X-ray...
We report the detection of [Ne II] emission at 12.81 μm in four out of the six optically thick dust ...
There is now a substantial body of evidence that disk-like structures of gas and dust surround many ...
Context. Anomalies in the abundance measurements of short lived radionuclides in meteorites indicate...