The analysis of the Advanced Satellite for Cosmology and Astrophysics (ASCA) spectra of the cool star binary system Capella is reported. The results of EUVE analysis, ASCA analysis, application of EUVE model to ASCA analysis, and Uncertainty Analysis are discussed
We present a SAX/LECS X-ray observation of the active binary Capella, the first coronal source obser...
In this paper we present a detailed analysis of two X-ray spectra of Capella, taken eleven months ap...
The binary star alpha Aurigae (otherwise known as Capella) is extremely important to understand the ...
The extreme ultraviolet (EUV) spectroscopy of several binary stars containing cool components is use...
Abstract. We present the high-resolution RGS X-ray spectrum of the stellar binary Capella observed b...
A list of publications and presentations supported by the NASA Grant, and copies of two of the paper...
International audienceWe present the high-resolution RGS X-ray spectrum of the stellar binary Capell...
We present the high-resolution RGS X-ray spectrum of the stellar binary Capella observed by the XMM-...
Context. Capella is among the few binary stars with two evolved giant components. The hotter compone...
Knowledge of the chemical composition and absolute masses of Capella are key to understanding the ev...
Received...; accepted... Context. Capella is among the few binary stars with two evolved giant compo...
In this paper we present a detailed analysis of two X-ray spectra of Capella, taken eleven months ap...
EUVE, ASCA, and XTE observed the eclipsing binary Algol (Beta Per) from 1-7 Feb. 96. The coordinated...
The solid state spectrometer on the Einstein Observatory determined .4 - 4.5 keV spectra for Capella...
We present a combined analysis of the X-ray emission of the Capella corona obtained with XMM-Newton ...
We present a SAX/LECS X-ray observation of the active binary Capella, the first coronal source obser...
In this paper we present a detailed analysis of two X-ray spectra of Capella, taken eleven months ap...
The binary star alpha Aurigae (otherwise known as Capella) is extremely important to understand the ...
The extreme ultraviolet (EUV) spectroscopy of several binary stars containing cool components is use...
Abstract. We present the high-resolution RGS X-ray spectrum of the stellar binary Capella observed b...
A list of publications and presentations supported by the NASA Grant, and copies of two of the paper...
International audienceWe present the high-resolution RGS X-ray spectrum of the stellar binary Capell...
We present the high-resolution RGS X-ray spectrum of the stellar binary Capella observed by the XMM-...
Context. Capella is among the few binary stars with two evolved giant components. The hotter compone...
Knowledge of the chemical composition and absolute masses of Capella are key to understanding the ev...
Received...; accepted... Context. Capella is among the few binary stars with two evolved giant compo...
In this paper we present a detailed analysis of two X-ray spectra of Capella, taken eleven months ap...
EUVE, ASCA, and XTE observed the eclipsing binary Algol (Beta Per) from 1-7 Feb. 96. The coordinated...
The solid state spectrometer on the Einstein Observatory determined .4 - 4.5 keV spectra for Capella...
We present a combined analysis of the X-ray emission of the Capella corona obtained with XMM-Newton ...
We present a SAX/LECS X-ray observation of the active binary Capella, the first coronal source obser...
In this paper we present a detailed analysis of two X-ray spectra of Capella, taken eleven months ap...
The binary star alpha Aurigae (otherwise known as Capella) is extremely important to understand the ...