activity
20152025
most citedCloud Formation and Acceleration in a Radiative Environment

36 citations · 99 across the 8 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

16 papers · 1 filter

astro-ph.GA2025

Oscillatory Line-Driven Winds: The Role of Atmospheric Stratification

Joshua Key, Daniel Proga, Randall Dannen +2

Time-dependent numerical studies of line-driven winds using the Sobolev approximation have a history spanning over three decades. In many of these studies, the wind solutions displ…

astro-ph.GA2024

AGN STORM 2: VIII. Investigating the Narrow Absorption Lines in Mrk 817 Using HST-COS Observations

Maryam Dehghanian, Nahum Arav, Gerard A. Kriss +39

We observed the Seyfert 1 galaxy Mrk817 during an intensive multi-wavelength reverberation mapping campaign for 16 months. Here, we examine the behavior of narrow UV absorption lin…

astro-ph.GA2024

Position dependent radiation fields near accretion disks

Kara Smith, Daniel Proga, Randall Dannen +2

In disk wind models for active galactic nuclei (AGN) outflows, high-energy radiation poses a significant problem wherein the gas can become overionized, effectively disabling what…

astro-ph.GA2023

AGN STORM 2: V. Anomalous Behavior of the CIV Light Curve in Mrk 817

Y. Homayouni, Gerard A. Kriss, Gisella De Rosa +49

An intensive reverberation mapping campaign on the Seyfert 1 galaxy Mrk817 using the Cosmic Origins Spectrograph (COS) on the Hubble Space Telescope (HST) revealed significant vari…

astro-ph.GA2023

On the transition from efficient to inefficient line-driving in irradiated flows

Randall Dannen, Daniel Proga, Tim Waters

Observations of ionized AGN outflows have provided compelling evidence that the radiation field transfers both momentum and energy to the plasma. At parsec scale distances in AGN,…

astro-ph.GA2021

On Synthetic Absorption Line Profiles of Thermally Driven Winds from Active Galactic Nuclei

Shalini Ganguly, Daniel Proga, Tim Waters +7

The warm absorbers observed in more than half of all nearby active galactic nuclei (AGN) are tracers of ionized outflows located at parsec scale distances from the central engine.…