The Galactic Center as a pradigm for low-luminosity nuclei? What can be learned from SgrA* for the central engine and conditions of star formation in nuclei of Seyfert galaxies and low luminosity nearby QSOs; The K-band identification of the DSO/G2 source from VLT and Keck data
A. Eckart*, S. Britzen, M. Horrobin, M. Zamaninasab, K. Muzic, N. Sabha,
B. Shahzamanian, S. Yazici, L. Moser, J. Zuther, M. Garcia-Marin, M. Valencia-S., M. Bursa, G. Karssen, V. Karas, B. Jalali, M. Vitale, M. Bremer, S. Fischer, S. Smajic, C. Rauch, D. Kunneriath, J. Moultaka, C. Straubmeier, Y.E. Rashed, C. Iserlohe, G. Busch, K. Markakis, A. Borkar and A. Zensuset al. (click to show)
Published on:
December 04, 2013
DOI: https://doi.org/10.22323/1.169.0004
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