Was 49b: An Overmassive AGN in a Merging Dwarf Galaxy?

We present a combined morphological and X-ray analysis of Was 49, an isolated, dual-AGN system notable for the presence of a dominant AGN, Was 49b, in the disk of the primary galaxy, Was 49a, at a projected radial distance of 8 kpc from the nucleus. Using X-ray data from Chandra, the Nuclear Spectro...

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Veröffentlicht in:	The Astrophysical journal 2017-02, Vol.836 (2), p.183
Hauptverfasser:	Secrest, Nathan J., Schmitt, Henrique R., Blecha, Laura, Rothberg, Barry, Fischer, Jacqueline
Format:	Artikel
Sprache:	eng
Schlagworte:	Active galactic nuclei Astrophysics ASTROPHYSICS, COSMOLOGY AND ASTRONOMY BLACK HOLES BOLOMETERS DISTANCE Dwarf galaxies Elliptical galaxies galaxies: active galaxies: bulges galaxies: dwarf galaxies: interactions galaxies: nuclei galaxies: Seyfert GALAXY NUCLEI INTERACTIONS LUMINOSITY MASS Morphology SEYFERT GALAXIES Space telescopes Spectroscopic telescopes Stars & galaxies Supermassive black holes TELESCOPES X RADIATION X ray analysis
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