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20102020
most citedX-ray Detected Active Galactic Nuclei in Dwarf Galaxies at

104 citations

Showing astro-ph.HEShow all

6 papers · 1 filter

astro-ph.HE2019★ 9 cited

Sub-Eddington super-massive black hole activity in Fornax early type galaxies

Nathan Lee, Elena Gallo, Edmund Hodges-Kluck +6

We characterize the incidence and intensity of low-level super-massive black hole activity within the Fornax cluster, through X-ray observations of the nuclei of 29 quiescent early…

astro-ph.HE2018★ 33 cited

Investigating the X-ray enhancements of highly radio-loud quasars at z > 4

Shifu Zhu, William N. Brandt, Jianfeng Wu +2

We have investigated the jet-linked \mbox{X-ray} emission from highly radio-loud quasars (HRLQs; ) at high redshift. We studied the X-ray properties of 15 HRLQs at $z>4…

astro-ph.HE2017★ 18 cited

AGN Activity in Nucleated Galaxies as Measured by Chandra

Adi Foord, Elena Gallo, Edmund Hodges-Kluck +4

Motivated by theoretical expectations that Nuclear Star Clusters (NSCs) in galactic centers may provide a favorable environment for super-massive black holes to form and/or efficie…

astro-ph.HE2016★ 14 cited

The X-ray Properties of Million Solar Mass Black Holes

Richard M. Plotkin, Elena Gallo, Francesco Haardt +5

We present new Chandra X-ray observations of seven low-mass black holes (~1e6 Msun) accreting at low Eddington ratios between -2.0<log L/Ledd<-1.5. We compare the X-ray properties…

astro-ph.HE2015

Ultraviolet/X-ray variability and the extended X-ray emission of the radio-loud broad absorption line quasar PG 1004+130

A. E. Scott, W. N. Brandt, B. P. Miller +2

We present the results of recent Chandra, XMM-Newton, and Hubble Space Telescope observations of the radio-loud (RL), broad absorption line (BAL) quasar PG 1004+130. We compare our…

astro-ph.HE2014★ 78 cited

A comprehensive statistical assessment of star-planet interaction

Brendan P. Miller, Elena Gallo, Jason T. Wright +1

We investigate whether magnetic interaction between close-in giant planets and their host stars produce observable statistical enhancements in stellar coronal or chromospheric acti…