activity
20162026
most citedA 10,000-solar-mass black hole in the nucleus of a bulgeless dwarf galaxy

79 citations · 676 across the 64 of their papers we have counts for

collaborators
Showing 2019 · astro-ph.GAShow all

6 papers · 2 filters

astro-ph.GA2019★ 20 cited

The Seoul National University AGN monitoring project. II. BLR size and black hole mass of two AGNs

Suvendu Rakshit, Jong-Hak Woo, Elena Gallo +20

Active galactic nuclei (AGNs) show a correlation between the size of the broad line region (BLR) and the monochromatic continuum luminosity at 5100 Å, allowing black hole mass esti…

astro-ph.GA2019★ 79 cited

A 10,000-solar-mass black hole in the nucleus of a bulgeless dwarf galaxy

Jong-Hak Woo, Hojin Cho, Elena Gallo +5

The motions of gas and stars in the nuclei of nearby large galaxies have demonstrated that massive black holes are common and that their masses strongly correlate with the stellar…

astro-ph.GA2019★ 16 cited

{\it HST}/COS Observations of the Warm Ionized Gaseous Halo of NGC 891

Zhijie Qu, Joel N. Bregman, Edmund J. Hodges-Kluck

The metallicity of galactic gaseous halos provides insights into accretion and feedback of galaxies. The nearby edge-on galaxy NGC 891 has a multi-component gaseous halo and a back…

astro-ph.GA2019★ 1 cited

A Survey of Hot Gas in the Universe

Joel N. Bregman, Edmund Hodges-Kluck, Benjamin D. Oppenheimer +8

A large fraction of the baryons and most of the metals in the Universe are unaccounted for. They likely lie in extended galaxy halos, galaxy groups, and the cosmic web, and measuri…

astro-ph.GA2019

Astro2020: How does dust escape from galaxies?

Edmund Hodges-Kluck, Lía Corrales, Sylvain Veilleux +3

Whenever gas is blown out of a galaxy, chances are that it contains some cosmic dust. This dust is an important part of the metals budget for the circumgalactic and intergalactic m…

astro-ph.GA2019

Astro2020: Hot Drivers of Stellar Feedback from 10 to 10,000 pc

Edmund Hodges-Kluck, Laura A. Lopez, Mihoko Yukita +5

Stellar feedback -- stars regulating further star formation through the injection of energy and momentum into the interstellar medium -- operates through a complex set of processes…