X-ray activities in the Galactic Center region. Maeda, Y., Koyama, K., Imanishi, K., Murakami, H., Nishiuchi, M., Sakano, M., Tsujimoto, M., Yokogawa, J., & Yamauchi, S. Astronomische Nachrichten, 320(4-5):177-178, 1999. ![X-ray activities in the Galactic Center region [link]](https://bibbase.org/img/filetypes/link.svg "link")
Website abstract bibtex With ASCA, we obtained detailed X-ray images and spectra of the Galactic Center. X-rays in the central parsecs from the dynamical center of the Galaxy, Sgr A*, were dominated by extended emission. Since Sgr A* was not spatially resolved from the extended structure, an upper limit to its luminosity was found to be 3 × 1035 erg s-1. This result indicates that the current AGN activity of the Galactic nucleus is very low. In the central hundreds of parsecs, X-ray stars, thin thermal diffuse plasma, and iron fluorescent emission from molecular clouds were seen. Based on the analyses of the X-ray stars and both of the diffuse components, we discuss some features which are possibly related to past nuclear activities.
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title = {X-ray activities in the Galactic Center region},
type = {article},
year = {1999},
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abstract = {With ASCA, we obtained detailed X-ray images and spectra of the Galactic Center. X-rays in the central parsecs from the dynamical center of the Galaxy, Sgr A*, were dominated by extended emission. Since Sgr A* was not spatially resolved from the extended structure, an upper limit to its luminosity was found to be 3 × 1035 erg s-1. This result indicates that the current AGN activity of the Galactic nucleus is very low. In the central hundreds of parsecs, X-ray stars, thin thermal diffuse plasma, and iron fluorescent emission from molecular clouds were seen. Based on the analyses of the X-ray stars and both of the diffuse components, we discuss some features which are possibly related to past nuclear activities.},
bibtype = {article},
author = {Maeda, Y. and Koyama, K. and Imanishi, K. and Murakami, H. and Nishiuchi, M. and Sakano, M. and Tsujimoto, M. and Yokogawa, J. and Yamauchi, S.},
journal = {Astronomische Nachrichten},
number = {4-5}
}
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