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22 papers
Star formation in quasar hosts and the origin of radio emission in radio-quiet quasars
Nadia L. Zakamska, Kelly Lampayan, Andreea Petric +11
Radio emission from radio-quiet quasars may be due to star formation in the quasar host galaxy, to a jet launched by the supermassive black hole, or to relativistic particles accel…
Multiwavelength View of the Inner Spiral of NGC 1365
I. V. Strateva, S. Komossa
We study the extended nuclear emission of the starburst galaxy NGC 1365. A weak obscured AGN and a strong starburst both contribute to the observed X-ray, optical, infrared, and ra…
Discovery of the Most-Distant Double-Peaked Emitter at z=1.369
B. Luo, W. N. Brandt, J. D. Silverman +10
We report the discovery of the most-distant double-peaked emitter, CXOECDFS J033115.0-275518, at z=1.369. A Keck/DEIMOS spectrum shows a clearly double-peaked broad Mg II $\lambda2…
The X-Ray Point-Source Population of NGC 1365: The Puzzle of Two Highly-Variable Ultraluminous X-ray Sources
Iskra V. Strateva, Stefanie Komossa
We present 26 point-sources discovered with Chandra within 200" (~20kpc) of the center of the barred supergiant galaxy NGC 1365. The majority of these sources are high-mass X-ray b…
A Chandra Look at Five of the Broadest Double-Peaked Balmer-Line Emitters
Iskra V. Strateva, W. N. Brandt, Michael Eracleous +1
We study the 0.5-10keV emission of a sample of five of the broadest double-peaked Balmer-line emitters with Chandra. The Balmer lines of these objects originate close (within a few…
The Spectral Energy Distributions of AGN with Double-Peaked Balmer Lines
I. Strateva, W. N. Brandt, M. Eracleous +2
We summarize the optical, UV, and X-ray properties of double-peaked emitters -- AGN with double-peaked Balmer emission lines believed to originate in the AGN accretion disk. We foc…