We review the properties of the variable X-ray emission from the extremely massive star Eta Carinae concentrating on the last X-ray minimum, and briefly consider the possible role of a binary companion star on the observational properties of the system
The campaign observations of the evolved super massive binary system, η Car, revealed an apparently ...
Context: If relativistic particle acceleration takes place in colliding-wind binaries, hard X-rays a...
Asymmetric variability in ultraviolet images of the Homunculus obtained with the Advanced Camera for...
We report the results of an X-ray observing campaign on the massive, evolved star Eta Carinae, conce...
The exceptional binary star Eta Carinae has been fascinating scientists and the people in the Southe...
It is believed that eta Carinae is actually a massive binary system, with the wind-wind interaction ...
X-ray emission from the supermassive star Eta Carinae (\ec) originates from hot shocked gas produced...
Abstract. We have investigated with BeppoSAX the long term behaviour of the harder X-ray component o...
Eta Carinae (eta Car) is a stellar binary system with a period of 5.54 years. It harbors one of the ...
We present the results of extensive observations by the gamma-ray AGILE satellite of the Galactic re...
We present XMM-Newton observations of the luminous star Eta Carinae, including a high resolution sof...
We present X-ray spectral fits to a recently obtained Chandra grating spectrum of Eta Carinae, one o...
An 85-day periodicity in the X-ray emission of Eta Carinae has been reported, while spectrocopic eve...
eta Carinae is a binary system formed by two massive stars, loosing mass through strong winds. The w...
Nearly all types of massive stars are known to display X-ray emission at some level. Tremendous insi...
The campaign observations of the evolved super massive binary system, η Car, revealed an apparently ...
Context: If relativistic particle acceleration takes place in colliding-wind binaries, hard X-rays a...
Asymmetric variability in ultraviolet images of the Homunculus obtained with the Advanced Camera for...
We report the results of an X-ray observing campaign on the massive, evolved star Eta Carinae, conce...
The exceptional binary star Eta Carinae has been fascinating scientists and the people in the Southe...
It is believed that eta Carinae is actually a massive binary system, with the wind-wind interaction ...
X-ray emission from the supermassive star Eta Carinae (\ec) originates from hot shocked gas produced...
Abstract. We have investigated with BeppoSAX the long term behaviour of the harder X-ray component o...
Eta Carinae (eta Car) is a stellar binary system with a period of 5.54 years. It harbors one of the ...
We present the results of extensive observations by the gamma-ray AGILE satellite of the Galactic re...
We present XMM-Newton observations of the luminous star Eta Carinae, including a high resolution sof...
We present X-ray spectral fits to a recently obtained Chandra grating spectrum of Eta Carinae, one o...
An 85-day periodicity in the X-ray emission of Eta Carinae has been reported, while spectrocopic eve...
eta Carinae is a binary system formed by two massive stars, loosing mass through strong winds. The w...
Nearly all types of massive stars are known to display X-ray emission at some level. Tremendous insi...
The campaign observations of the evolved super massive binary system, η Car, revealed an apparently ...
Context: If relativistic particle acceleration takes place in colliding-wind binaries, hard X-rays a...
Asymmetric variability in ultraviolet images of the Homunculus obtained with the Advanced Camera for...